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The Diagnosis: Hypertrophic Lichen Planus

Two biopsies from the left lateral foot revealed hyperkeratosis, wedge-shaped hypergranulosis, irregular acanthosis, and a bandlike lymphocytic infiltrate in the superficial dermis with a classic sawtooth pattern of the rete ridges (Figure 1). Based on the clinical findings and histopathology, the patient was diagnosed with hypertrophic lichen planus (LP) and was treated with clobetasol ointment 0.05%, which resulted in progression of the symptoms. She experienced notable improvement 3 months after adding methotrexate 12.5 mg weekly (Figure 2).

Lichen planus is an idiopathic chronic inflammatory condition of the skin and mucous membranes that classically manifests as pruritic violaceous papules and plaques, which commonly are found on the wrists, lower back, and ankles.¹ The most common variants of LP are hypertrophic, linear, mucosal, actinic, follicular, pigmented, annular, atrophic, and guttate.² The clinical presentation and biopsy results in our patient were consistent with the hypertrophic variant of LP, which is a chronic condition that most often manifests on the lower legs, especially around the ankles, as hyperkeratotic papules, plaques, and nodules.^2,3 The exact pathophysiology of hypertrophic LP is unknown, but there is evidence that the immune system plays a role in its development and that the Koebner phenomenon may contribute to its exacerbation.⁴ There is a well-known association between LP and hepatitis. Patients with chronic LP may develop squamous cell carcinoma.⁴ The variants of LP can overlap and do not exist independent of one another. Recognizing the overlap in these variants allows for earlier diagnosis and therapeutic intervention of the disease process to limit disease progression and patient clinic visits and to improve patient quality of life.

The differential diagnosis for hyperkeratotic plaques of the feet and ankles can be broad and may include keratosis lichenoides chronica, palmoplantar keratoderma, palmoplantar psoriasis, or lichen amyloidosis. These conditions are classified based on various criteria that include extent of disease manifestations, morphology of palmoplantar skin involvement, inheritance patterns, and molecular pathogenesis.⁵ Keratosis lichenoides chronica is a rare dermatosis that presents as a distinctive seborrheic dermatitis–like facial eruption. The facial eruption is accompanied by violaceous papular and nodular lesions that appear on the extremities and trunk, typically arranged in a linear or reticular pattern.⁶ Palmoplantar keratoderma represents a group of acquired and hereditary conditions that are characterized by excessive thickening of the palms and soles.⁵ Palmoplantar psoriasis is a variant of psoriasis that affects the palms and soles and can manifest as hyperkeratosis, pustular, or mixed morphology.⁷ Lichen amyloidosis is a subtype of primary localized cutaneous amyloidosis that manifests as multiple pruritic, firm, hyperpigmented, hyperkeratotic papules on the shins that later coalesce in a rippled pattern.^8,9

The first-line treatment for hypertrophic LP is topical corticosteroids. Alternative therapies include mycophenolate mofetil, acitretin, and intralesional corticosteroid injections.⁴ Treatment is similar for all of the LP variants.

The Diagnosis: Hypertrophic Lichen Planus

Two biopsies from the left lateral foot revealed hyperkeratosis, wedge-shaped hypergranulosis, irregular acanthosis, and a bandlike lymphocytic infiltrate in the superficial dermis with a classic sawtooth pattern of the rete ridges (Figure 1). Based on the clinical findings and histopathology, the patient was diagnosed with hypertrophic lichen planus (LP) and was treated with clobetasol ointment 0.05%, which resulted in progression of the symptoms. She experienced notable improvement 3 months after adding methotrexate 12.5 mg weekly (Figure 2).

Lichen planus is an idiopathic chronic inflammatory condition of the skin and mucous membranes that classically manifests as pruritic violaceous papules and plaques, which commonly are found on the wrists, lower back, and ankles.¹ The most common variants of LP are hypertrophic, linear, mucosal, actinic, follicular, pigmented, annular, atrophic, and guttate.² The clinical presentation and biopsy results in our patient were consistent with the hypertrophic variant of LP, which is a chronic condition that most often manifests on the lower legs, especially around the ankles, as hyperkeratotic papules, plaques, and nodules.^2,3 The exact pathophysiology of hypertrophic LP is unknown, but there is evidence that the immune system plays a role in its development and that the Koebner phenomenon may contribute to its exacerbation.⁴ There is a well-known association between LP and hepatitis. Patients with chronic LP may develop squamous cell carcinoma.⁴ The variants of LP can overlap and do not exist independent of one another. Recognizing the overlap in these variants allows for earlier diagnosis and therapeutic intervention of the disease process to limit disease progression and patient clinic visits and to improve patient quality of life.

The differential diagnosis for hyperkeratotic plaques of the feet and ankles can be broad and may include keratosis lichenoides chronica, palmoplantar keratoderma, palmoplantar psoriasis, or lichen amyloidosis. These conditions are classified based on various criteria that include extent of disease manifestations, morphology of palmoplantar skin involvement, inheritance patterns, and molecular pathogenesis.⁵ Keratosis lichenoides chronica is a rare dermatosis that presents as a distinctive seborrheic dermatitis–like facial eruption. The facial eruption is accompanied by violaceous papular and nodular lesions that appear on the extremities and trunk, typically arranged in a linear or reticular pattern.⁶ Palmoplantar keratoderma represents a group of acquired and hereditary conditions that are characterized by excessive thickening of the palms and soles.⁵ Palmoplantar psoriasis is a variant of psoriasis that affects the palms and soles and can manifest as hyperkeratosis, pustular, or mixed morphology.⁷ Lichen amyloidosis is a subtype of primary localized cutaneous amyloidosis that manifests as multiple pruritic, firm, hyperpigmented, hyperkeratotic papules on the shins that later coalesce in a rippled pattern.^8,9

The first-line treatment for hypertrophic LP is topical corticosteroids. Alternative therapies include mycophenolate mofetil, acitretin, and intralesional corticosteroid injections.⁴ Treatment is similar for all of the LP variants.

The Diagnosis: Hypertrophic Lichen Planus

Two biopsies from the left lateral foot revealed hyperkeratosis, wedge-shaped hypergranulosis, irregular acanthosis, and a bandlike lymphocytic infiltrate in the superficial dermis with a classic sawtooth pattern of the rete ridges (Figure 1). Based on the clinical findings and histopathology, the patient was diagnosed with hypertrophic lichen planus (LP) and was treated with clobetasol ointment 0.05%, which resulted in progression of the symptoms. She experienced notable improvement 3 months after adding methotrexate 12.5 mg weekly (Figure 2).

Lichen planus is an idiopathic chronic inflammatory condition of the skin and mucous membranes that classically manifests as pruritic violaceous papules and plaques, which commonly are found on the wrists, lower back, and ankles.¹ The most common variants of LP are hypertrophic, linear, mucosal, actinic, follicular, pigmented, annular, atrophic, and guttate.² The clinical presentation and biopsy results in our patient were consistent with the hypertrophic variant of LP, which is a chronic condition that most often manifests on the lower legs, especially around the ankles, as hyperkeratotic papules, plaques, and nodules.^2,3 The exact pathophysiology of hypertrophic LP is unknown, but there is evidence that the immune system plays a role in its development and that the Koebner phenomenon may contribute to its exacerbation.⁴ There is a well-known association between LP and hepatitis. Patients with chronic LP may develop squamous cell carcinoma.⁴ The variants of LP can overlap and do not exist independent of one another. Recognizing the overlap in these variants allows for earlier diagnosis and therapeutic intervention of the disease process to limit disease progression and patient clinic visits and to improve patient quality of life.

The differential diagnosis for hyperkeratotic plaques of the feet and ankles can be broad and may include keratosis lichenoides chronica, palmoplantar keratoderma, palmoplantar psoriasis, or lichen amyloidosis. These conditions are classified based on various criteria that include extent of disease manifestations, morphology of palmoplantar skin involvement, inheritance patterns, and molecular pathogenesis.⁵ Keratosis lichenoides chronica is a rare dermatosis that presents as a distinctive seborrheic dermatitis–like facial eruption. The facial eruption is accompanied by violaceous papular and nodular lesions that appear on the extremities and trunk, typically arranged in a linear or reticular pattern.⁶ Palmoplantar keratoderma represents a group of acquired and hereditary conditions that are characterized by excessive thickening of the palms and soles.⁵ Palmoplantar psoriasis is a variant of psoriasis that affects the palms and soles and can manifest as hyperkeratosis, pustular, or mixed morphology.⁷ Lichen amyloidosis is a subtype of primary localized cutaneous amyloidosis that manifests as multiple pruritic, firm, hyperpigmented, hyperkeratotic papules on the shins that later coalesce in a rippled pattern.^8,9

The first-line treatment for hypertrophic LP is topical corticosteroids. Alternative therapies include mycophenolate mofetil, acitretin, and intralesional corticosteroid injections.⁴ Treatment is similar for all of the LP variants.

The Diagnosis: Lymphoepithelioma-like Carcinoma

Lymphoepithelioma-like carcinoma (LELC) is a rare, poorly differentiated, primary cutaneous neoplasm that occurs on sun-exposed skin, particularly on the head and neck of elderly individuals. It often manifests as an asymptomatic, slow-growing, flesh-colored or erythematous dermal nodule, though ulceration and tenderness have been reported.¹ Histopathologically, these neoplasms often are poorly circumscribed and can infiltrate surrounding subcutaneous and soft tissue. As a biphasic tumor, LELC is characterized by islands, nests, or trabeculae of epithelioid cells within the mid dermis surrounded by a dense lymphocytic infiltrate with plasma cells (Figure 1).¹ The epithelial component rarely communicates with the overlying epidermis and is composed of atypical polygonal cells with eosinophilic cytoplasm, vesicular nuclei, prominent nucleoli, and frequent mitosis.² These epithelial nests can be highlighted by pancytokeratin AE1/AE3 or other epithelial differentiation markers (eg, CAM 5.2, CK5/6, epithelial membrane antigen, high-molecular-weight cytokeratin), while the surrounding lymphocytic infiltrate consists of an admixture of T cells and B cells. Lymphoepithelioma-like carcinomas also can demonstrate sebaceous, eccrine, or follicular differentiations.³ The epithelial nests of LELC also are positive for p63 and epithelial membrane antigen.²

The usual treatment of LELC is wide local excision or Mohs micrographic surgery.¹ Despite the poorly differentiated morphology of the tumor, LELC has a generally good prognosis with low metastatic potential and few reports of local recurrence after incomplete excision.³ Patients who are not candidates for surgery as well as recalcitrant cases are managed with radiotherapy.¹

Cutaneous lymphadenoma (CL) is a benign adnexal neoplasm that manifests as a small, solitary, fleshcolored nodule usually in the head and neck region.⁴ Histologically, CL consists of well-circumscribed epithelial nests within the dermis that are peripherally outlined by palisading basaloid cells and filled with clear to eosinophilic epithelioid cells (Figure 2).5 The fibrotic tumor stroma often is infiltrated by numerous intralobular dendritic cells and lymphocytes that occasionally can be arranged in germinal center–like nodules.⁴ The lymphoepithelial nature of CL can be challenging to distinguish morphologically from LELC, and immunohistochemistry stains may be required. In CL, both the basaloid and epithelioid cells stain positive for pancytokeratin AE1/ AE3, but the peripheral palisaded basaloid cells also stain positive for BerEP4. Additionally, the fibrotic stroma can be highlighted by CD34 and the intralobular dendritic cells by S-100.⁴

Nasopharyngeal carcinoma (NPC), formerly known as lymphoepithelioma, refers to carcinoma arising within the epithelium of the nasopharynx.⁶ Endemic to China, NPC manifests as an enlarging nasopharyngeal mass, causing clinical symptoms such as nasal obstruction and epistaxis.⁷ Histologically, nonkeratinizing NPC exhibits a biphasic morphology consisting of epithelioid neoplastic cells and background lymphocytic infiltrates (Figure 3). The epithelial component consists of round to oval neoplastic cells with amphophilic to eosinophilic cytoplasm, vesicular nuclei, and prominent nucleoli.⁶ Nasopharyngeal carcinoma is associated strongly with the Epstein-Barr virus while LELC is not; thus, Epstein- Barr encoding region in situ hybridization can reliably distinguish these entities. Metastatic NPC is rare but has been reported; therefore, it is highly recommended to perform an otolaryngologic examination in addition to testing for Epstein-Barr virus reactivity as part of a complete evaluation.⁸

Cutaneous squamous cell carcinoma (SCC) is a common epidermal malignancy with multiple subtypes and variable morphology. The clinical presentation of SCC is similar to LELC—an enlarging hyperkeratotic papule or nodule on sun-exposed skin that often is ulcerated and tender.⁹ Histologically, poorly differentiated nonkeratinizing SCC can form nests and trabeculae of epithelioid cells that are stained by epithelial differentiation markers, resembling the epithelioid nests of LELC. Distinguishing between LELC and poorly differentiated SCC with robust inflammatory infiltrate can be challenging (Figure 4). In fact, some experts support LELC as an SCC variant rather than a separate entity.9 However, in contrast to LELC, the dermal nests of SCC usually maintain an epidermal connection and often are associated with an overlying area of SCC in situ or welldifferentiated SCC.³

Mycosis fungoides (MF) is a primary cutaneous T-cell lymphoma. It is the most common type of cutaneous lymphoma, accounting for almost 50% of all reported cases.¹⁰ Classic MF has an indolent course and progresses through several clinical stages. Patches and plaques characterize early stages; lymphadenopathy indicates progression to later stages in which erythroderma may develop with coalescence of patches, plaques, and tumors; and MF present in blood or lymph nodes characterizes the late stage. Each stage of MF is different histologically—from a superficial lichenoid infiltrate with exocytosis of malignant T cells in the patch stage, to more robust epidermotropism and dermal infiltrate in the plaque stage, and finally a dense dermal infiltrate in the late stage.¹¹ The rare syringotropic variant of MF clinically manifests as solitary or multiple erythematous lesions, often with overlying alopecia. Syringotropic MF uniquely exhibits folliculotropism and syringotropism along with syringometaplasia on histologic evaluation (Figure 5).¹² The syringometaplasia can be difficult to distinguish from the epithelial nests of LELC, particularly with the lymphocytic background. Immunohistochemical panels for T-cell markers can highlight aberrant T cells in syringotropic MF through their usual loss of CD5 and CD7, in comparison to normal T cells in LELC.¹¹ An elevated CD4:CD8 ratio of 4:1 and molecular analysis for T-cell receptor gene clonal rearrangements also can support the diagnosis of MF.¹²

The Diagnosis: Lymphoepithelioma-like Carcinoma

Lymphoepithelioma-like carcinoma (LELC) is a rare, poorly differentiated, primary cutaneous neoplasm that occurs on sun-exposed skin, particularly on the head and neck of elderly individuals. It often manifests as an asymptomatic, slow-growing, flesh-colored or erythematous dermal nodule, though ulceration and tenderness have been reported.¹ Histopathologically, these neoplasms often are poorly circumscribed and can infiltrate surrounding subcutaneous and soft tissue. As a biphasic tumor, LELC is characterized by islands, nests, or trabeculae of epithelioid cells within the mid dermis surrounded by a dense lymphocytic infiltrate with plasma cells (Figure 1).¹ The epithelial component rarely communicates with the overlying epidermis and is composed of atypical polygonal cells with eosinophilic cytoplasm, vesicular nuclei, prominent nucleoli, and frequent mitosis.² These epithelial nests can be highlighted by pancytokeratin AE1/AE3 or other epithelial differentiation markers (eg, CAM 5.2, CK5/6, epithelial membrane antigen, high-molecular-weight cytokeratin), while the surrounding lymphocytic infiltrate consists of an admixture of T cells and B cells. Lymphoepithelioma-like carcinomas also can demonstrate sebaceous, eccrine, or follicular differentiations.³ The epithelial nests of LELC also are positive for p63 and epithelial membrane antigen.²

The usual treatment of LELC is wide local excision or Mohs micrographic surgery.¹ Despite the poorly differentiated morphology of the tumor, LELC has a generally good prognosis with low metastatic potential and few reports of local recurrence after incomplete excision.³ Patients who are not candidates for surgery as well as recalcitrant cases are managed with radiotherapy.¹

Cutaneous lymphadenoma (CL) is a benign adnexal neoplasm that manifests as a small, solitary, fleshcolored nodule usually in the head and neck region.⁴ Histologically, CL consists of well-circumscribed epithelial nests within the dermis that are peripherally outlined by palisading basaloid cells and filled with clear to eosinophilic epithelioid cells (Figure 2).5 The fibrotic tumor stroma often is infiltrated by numerous intralobular dendritic cells and lymphocytes that occasionally can be arranged in germinal center–like nodules.⁴ The lymphoepithelial nature of CL can be challenging to distinguish morphologically from LELC, and immunohistochemistry stains may be required. In CL, both the basaloid and epithelioid cells stain positive for pancytokeratin AE1/ AE3, but the peripheral palisaded basaloid cells also stain positive for BerEP4. Additionally, the fibrotic stroma can be highlighted by CD34 and the intralobular dendritic cells by S-100.⁴

Nasopharyngeal carcinoma (NPC), formerly known as lymphoepithelioma, refers to carcinoma arising within the epithelium of the nasopharynx.⁶ Endemic to China, NPC manifests as an enlarging nasopharyngeal mass, causing clinical symptoms such as nasal obstruction and epistaxis.⁷ Histologically, nonkeratinizing NPC exhibits a biphasic morphology consisting of epithelioid neoplastic cells and background lymphocytic infiltrates (Figure 3). The epithelial component consists of round to oval neoplastic cells with amphophilic to eosinophilic cytoplasm, vesicular nuclei, and prominent nucleoli.⁶ Nasopharyngeal carcinoma is associated strongly with the Epstein-Barr virus while LELC is not; thus, Epstein- Barr encoding region in situ hybridization can reliably distinguish these entities. Metastatic NPC is rare but has been reported; therefore, it is highly recommended to perform an otolaryngologic examination in addition to testing for Epstein-Barr virus reactivity as part of a complete evaluation.⁸

Cutaneous squamous cell carcinoma (SCC) is a common epidermal malignancy with multiple subtypes and variable morphology. The clinical presentation of SCC is similar to LELC—an enlarging hyperkeratotic papule or nodule on sun-exposed skin that often is ulcerated and tender.⁹ Histologically, poorly differentiated nonkeratinizing SCC can form nests and trabeculae of epithelioid cells that are stained by epithelial differentiation markers, resembling the epithelioid nests of LELC. Distinguishing between LELC and poorly differentiated SCC with robust inflammatory infiltrate can be challenging (Figure 4). In fact, some experts support LELC as an SCC variant rather than a separate entity.9 However, in contrast to LELC, the dermal nests of SCC usually maintain an epidermal connection and often are associated with an overlying area of SCC in situ or welldifferentiated SCC.³

Mycosis fungoides (MF) is a primary cutaneous T-cell lymphoma. It is the most common type of cutaneous lymphoma, accounting for almost 50% of all reported cases.¹⁰ Classic MF has an indolent course and progresses through several clinical stages. Patches and plaques characterize early stages; lymphadenopathy indicates progression to later stages in which erythroderma may develop with coalescence of patches, plaques, and tumors; and MF present in blood or lymph nodes characterizes the late stage. Each stage of MF is different histologically—from a superficial lichenoid infiltrate with exocytosis of malignant T cells in the patch stage, to more robust epidermotropism and dermal infiltrate in the plaque stage, and finally a dense dermal infiltrate in the late stage.¹¹ The rare syringotropic variant of MF clinically manifests as solitary or multiple erythematous lesions, often with overlying alopecia. Syringotropic MF uniquely exhibits folliculotropism and syringotropism along with syringometaplasia on histologic evaluation (Figure 5).¹² The syringometaplasia can be difficult to distinguish from the epithelial nests of LELC, particularly with the lymphocytic background. Immunohistochemical panels for T-cell markers can highlight aberrant T cells in syringotropic MF through their usual loss of CD5 and CD7, in comparison to normal T cells in LELC.¹¹ An elevated CD4:CD8 ratio of 4:1 and molecular analysis for T-cell receptor gene clonal rearrangements also can support the diagnosis of MF.¹²

The Diagnosis: Lymphoepithelioma-like Carcinoma

Lymphoepithelioma-like carcinoma (LELC) is a rare, poorly differentiated, primary cutaneous neoplasm that occurs on sun-exposed skin, particularly on the head and neck of elderly individuals. It often manifests as an asymptomatic, slow-growing, flesh-colored or erythematous dermal nodule, though ulceration and tenderness have been reported.¹ Histopathologically, these neoplasms often are poorly circumscribed and can infiltrate surrounding subcutaneous and soft tissue. As a biphasic tumor, LELC is characterized by islands, nests, or trabeculae of epithelioid cells within the mid dermis surrounded by a dense lymphocytic infiltrate with plasma cells (Figure 1).¹ The epithelial component rarely communicates with the overlying epidermis and is composed of atypical polygonal cells with eosinophilic cytoplasm, vesicular nuclei, prominent nucleoli, and frequent mitosis.² These epithelial nests can be highlighted by pancytokeratin AE1/AE3 or other epithelial differentiation markers (eg, CAM 5.2, CK5/6, epithelial membrane antigen, high-molecular-weight cytokeratin), while the surrounding lymphocytic infiltrate consists of an admixture of T cells and B cells. Lymphoepithelioma-like carcinomas also can demonstrate sebaceous, eccrine, or follicular differentiations.³ The epithelial nests of LELC also are positive for p63 and epithelial membrane antigen.²

The usual treatment of LELC is wide local excision or Mohs micrographic surgery.¹ Despite the poorly differentiated morphology of the tumor, LELC has a generally good prognosis with low metastatic potential and few reports of local recurrence after incomplete excision.³ Patients who are not candidates for surgery as well as recalcitrant cases are managed with radiotherapy.¹

Cutaneous lymphadenoma (CL) is a benign adnexal neoplasm that manifests as a small, solitary, fleshcolored nodule usually in the head and neck region.⁴ Histologically, CL consists of well-circumscribed epithelial nests within the dermis that are peripherally outlined by palisading basaloid cells and filled with clear to eosinophilic epithelioid cells (Figure 2).5 The fibrotic tumor stroma often is infiltrated by numerous intralobular dendritic cells and lymphocytes that occasionally can be arranged in germinal center–like nodules.⁴ The lymphoepithelial nature of CL can be challenging to distinguish morphologically from LELC, and immunohistochemistry stains may be required. In CL, both the basaloid and epithelioid cells stain positive for pancytokeratin AE1/ AE3, but the peripheral palisaded basaloid cells also stain positive for BerEP4. Additionally, the fibrotic stroma can be highlighted by CD34 and the intralobular dendritic cells by S-100.⁴

Nasopharyngeal carcinoma (NPC), formerly known as lymphoepithelioma, refers to carcinoma arising within the epithelium of the nasopharynx.⁶ Endemic to China, NPC manifests as an enlarging nasopharyngeal mass, causing clinical symptoms such as nasal obstruction and epistaxis.⁷ Histologically, nonkeratinizing NPC exhibits a biphasic morphology consisting of epithelioid neoplastic cells and background lymphocytic infiltrates (Figure 3). The epithelial component consists of round to oval neoplastic cells with amphophilic to eosinophilic cytoplasm, vesicular nuclei, and prominent nucleoli.⁶ Nasopharyngeal carcinoma is associated strongly with the Epstein-Barr virus while LELC is not; thus, Epstein- Barr encoding region in situ hybridization can reliably distinguish these entities. Metastatic NPC is rare but has been reported; therefore, it is highly recommended to perform an otolaryngologic examination in addition to testing for Epstein-Barr virus reactivity as part of a complete evaluation.⁸

Cutaneous squamous cell carcinoma (SCC) is a common epidermal malignancy with multiple subtypes and variable morphology. The clinical presentation of SCC is similar to LELC—an enlarging hyperkeratotic papule or nodule on sun-exposed skin that often is ulcerated and tender.⁹ Histologically, poorly differentiated nonkeratinizing SCC can form nests and trabeculae of epithelioid cells that are stained by epithelial differentiation markers, resembling the epithelioid nests of LELC. Distinguishing between LELC and poorly differentiated SCC with robust inflammatory infiltrate can be challenging (Figure 4). In fact, some experts support LELC as an SCC variant rather than a separate entity.9 However, in contrast to LELC, the dermal nests of SCC usually maintain an epidermal connection and often are associated with an overlying area of SCC in situ or welldifferentiated SCC.³

Mycosis fungoides (MF) is a primary cutaneous T-cell lymphoma. It is the most common type of cutaneous lymphoma, accounting for almost 50% of all reported cases.¹⁰ Classic MF has an indolent course and progresses through several clinical stages. Patches and plaques characterize early stages; lymphadenopathy indicates progression to later stages in which erythroderma may develop with coalescence of patches, plaques, and tumors; and MF present in blood or lymph nodes characterizes the late stage. Each stage of MF is different histologically—from a superficial lichenoid infiltrate with exocytosis of malignant T cells in the patch stage, to more robust epidermotropism and dermal infiltrate in the plaque stage, and finally a dense dermal infiltrate in the late stage.¹¹ The rare syringotropic variant of MF clinically manifests as solitary or multiple erythematous lesions, often with overlying alopecia. Syringotropic MF uniquely exhibits folliculotropism and syringotropism along with syringometaplasia on histologic evaluation (Figure 5).¹² The syringometaplasia can be difficult to distinguish from the epithelial nests of LELC, particularly with the lymphocytic background. Immunohistochemical panels for T-cell markers can highlight aberrant T cells in syringotropic MF through their usual loss of CD5 and CD7, in comparison to normal T cells in LELC.¹¹ An elevated CD4:CD8 ratio of 4:1 and molecular analysis for T-cell receptor gene clonal rearrangements also can support the diagnosis of MF.¹²

Plant Parts and Nomenclature

Ficus carica (common fig) is a deciduous shrub or small tree with smooth gray bark that can grow up to 10 m in height (Figure 1). It is characterized by many spreading branches, but the trunk rarely grows beyond a diameter of 7 in. Its hairy leaves are coarse on the upper side and soft underneath with 3 to 7 deep lobes that can extend up to 25 cm in length or width; the leaves grow individually, alternating along the sides of the branches. Fig trees often can be seen adorning yards, gardens, and parks, especially in tropical and subtropical climates. Ficus carica should not be confused with Ficus benjamina (weeping fig), a common ornamental tree that also is used to provide shade in hot climates, though both can cause phototoxic skin eruptions.

The common fig tree originated in the Mediterranean and western Asia¹ and has been cultivated by humans since the second and third millennia bc for its fruit, which commonly is used to sweeten cookies, cakes, and jams.² Figs are the most commonly mentioned food plant in the Bible, with at least 56 references in the Old and New Testaments.³ The “fruit” technically is a syconium—a hollow fleshy receptacle with a small opening at the apex partly closed by small scales. It can be obovoid, turbinate, or pear shaped; can be 1 to 4 inches long; and can vary in color from yellowish green to coppery, bronze, or dark purple (Figure 2).

Ficus carica is a member of the Moraceae family (derived from the Latin name for the mulberry tree), which includes 53 genera and approximately 1400 species, of which about 850 belong to the genus Ficus (the Latin name for a fig tree). The term carica likely comes from the Latin word carricare (to load) to describe a tree loaded with figs. Family members include trees, shrubs, lianas, and herbs that usually contain laticifers with a milky latex.

Traditional Uses

For centuries, components of the fig tree have been used in herbal teas and pastes to treat ailments ranging from sore throats to diarrhea, though there is no evidence to support their efficacy.⁴ Ancient Indians and Egyptians used plants such as the common fig tree containing furocoumarins to induce hyperpigmentation in vitiligo.⁵

Phototoxic Components

The leaves and sap of the common fig tree contain psoralens, which are members of the furocoumarin group of chemical compounds and are the source of its phototoxicity. The fruit does not contain psoralens.^6-9 The tree also produces proteolytic enzymes such as protease, amylase, ficin, triterpenoids, and lipodiastase that enhance its phototoxic effects.⁸ Exposure to UV light between 320 and 400 nm following contact with these phototoxic components triggers a reaction in the skin over the course of 1 to 3 days.⁵ The psoralens bind in epidermal cells, cross-link the DNA, and cause cell-membrane destruction, leading to edema and necrosis.¹⁰ The delay in symptoms may be attributed to the time needed to synthesize acute-phase reaction proteins such as tumor necrosis factor α and IL-1.¹¹ In spring and summer months, an increased concentration of psoralens in the leaves and sap contribute to an increased incidence of phytophotodermatitis.⁹ Humidity and sweat also increase the percutaneous absorption of psoralens.^12,13

Allergens

Fig trees produce a latex protein that can cause cross-reactive hypersensitivity reactions in those allergic to F benjamina latex and rubber latex.⁶ The latex proteins in fig trees can act as airborne respiratory allergens. Ingestion of figs can produce anaphylactic reactions in those sensitized to rubber latex and F benjamina latex.⁷ Other plant families associated with phototoxic reactions include Rutaceae (lemon, lime, bitter orange), Apiaceae (formerly Umbelliferae)(carrot, parsnip, parsley, dill, celery, hogweed), and Fabaceae (prairie turnip).

Most cases of fig phytophotodermatitis begin with burning, pain, and/or itching within hours of sunlight exposure in areas of the skin that encountered components of the fig tree, often in a linear pattern. The affected areas become erythematous and edematous with formation of bullae and unilocular vesicles over the course of 1 to 3 days.^12,14,15 Lesions may extend beyond the region of contact with the fig tree as they spread across the skin due to sweat or friction, and pain may linger even after the lesions resolve.^12,13,16 Adults who handle fig trees (eg, pruning) are susceptible to phototoxic reactions, especially those using chain saws or other mechanisms that result in spray exposure, as the photosensitizing sap permeates the wood and bark of the entire tree.¹⁷ Similarly, children who handle fig leaves or sap during outdoor play can develop bullous eruptions. Severe cases have resulted in hospital admission after prolonged exposure.¹⁶ Additionally, irritant dermatitis may arise from contact with the trichomes or “hairs” on various parts of the plant.

Image provided with permission by Scott Norton, MD, MPH, MSc (Washington, DC).

Patients who use natural remedies containing components of the fig tree without the supervision of a medical provider put themselves at risk for unsafe or unwanted adverse effects, such as phytophotodermatitis.^12,15,16,18 An entire family presented with burns after they applied fig leaf extract to the skin prior to tanning outside in the sun.¹⁹ A 42-year-old woman acquired a severe burn covering 81% of the body surface after topically applying fig leaf tea to the skin as a tanning agent.²⁰ A subset of patients ingesting or applying fig tree components for conditions such as vitiligo, dermatitis, onychomycosis, and motor retardation developed similar cutaneous reactions.^13,14,21,22 Lesions resembling finger marks can raise concerns for potential abuse or neglect in children.²²

The differential diagnosis for fig phytophotodermatitis includes sunburn, chemical burns, drug-related photosensitivity, infectious lesions (eg, herpes simplex, bullous impetigo, Lyme disease, superficial lymphangitis), connective tissue disease (eg, systemic lupus erythematosus), contact dermatitis, and nonaccidental trauma.^12,15,18 Compared to sunburn, phytophotodermatitis tends to increase in severity over days following exposure and heals with dramatic hyperpigmentation, which also prompts visits to dermatology.¹²

Treatment

Treatment of fig phytophotodermatitis chiefly is symptomatic, including analgesia, appropriate wound care, and infection prophylaxis. Topical and systemic corticosteroids may aid in the resolution of moderate to severe reactions.^15,23,24 Even severe injuries over small areas or mild injuries to a high percentage of the total body surface area may require treatment in a burn unit. Patients should be encouraged to use mineral-based sunscreens on the affected areas to reduce the risk for hyperpigmentation. Individuals who regularly handle fig trees should use contact barriers including gloves and protective clothing (eg, long-sleeved shirts, long pants).

Plant Parts and Nomenclature

Ficus carica (common fig) is a deciduous shrub or small tree with smooth gray bark that can grow up to 10 m in height (Figure 1). It is characterized by many spreading branches, but the trunk rarely grows beyond a diameter of 7 in. Its hairy leaves are coarse on the upper side and soft underneath with 3 to 7 deep lobes that can extend up to 25 cm in length or width; the leaves grow individually, alternating along the sides of the branches. Fig trees often can be seen adorning yards, gardens, and parks, especially in tropical and subtropical climates. Ficus carica should not be confused with Ficus benjamina (weeping fig), a common ornamental tree that also is used to provide shade in hot climates, though both can cause phototoxic skin eruptions.

The common fig tree originated in the Mediterranean and western Asia¹ and has been cultivated by humans since the second and third millennia bc for its fruit, which commonly is used to sweeten cookies, cakes, and jams.² Figs are the most commonly mentioned food plant in the Bible, with at least 56 references in the Old and New Testaments.³ The “fruit” technically is a syconium—a hollow fleshy receptacle with a small opening at the apex partly closed by small scales. It can be obovoid, turbinate, or pear shaped; can be 1 to 4 inches long; and can vary in color from yellowish green to coppery, bronze, or dark purple (Figure 2).

Ficus carica is a member of the Moraceae family (derived from the Latin name for the mulberry tree), which includes 53 genera and approximately 1400 species, of which about 850 belong to the genus Ficus (the Latin name for a fig tree). The term carica likely comes from the Latin word carricare (to load) to describe a tree loaded with figs. Family members include trees, shrubs, lianas, and herbs that usually contain laticifers with a milky latex.

Traditional Uses

For centuries, components of the fig tree have been used in herbal teas and pastes to treat ailments ranging from sore throats to diarrhea, though there is no evidence to support their efficacy.⁴ Ancient Indians and Egyptians used plants such as the common fig tree containing furocoumarins to induce hyperpigmentation in vitiligo.⁵

Phototoxic Components

The leaves and sap of the common fig tree contain psoralens, which are members of the furocoumarin group of chemical compounds and are the source of its phototoxicity. The fruit does not contain psoralens.^6-9 The tree also produces proteolytic enzymes such as protease, amylase, ficin, triterpenoids, and lipodiastase that enhance its phototoxic effects.⁸ Exposure to UV light between 320 and 400 nm following contact with these phototoxic components triggers a reaction in the skin over the course of 1 to 3 days.⁵ The psoralens bind in epidermal cells, cross-link the DNA, and cause cell-membrane destruction, leading to edema and necrosis.¹⁰ The delay in symptoms may be attributed to the time needed to synthesize acute-phase reaction proteins such as tumor necrosis factor α and IL-1.¹¹ In spring and summer months, an increased concentration of psoralens in the leaves and sap contribute to an increased incidence of phytophotodermatitis.⁹ Humidity and sweat also increase the percutaneous absorption of psoralens.^12,13

Allergens

Fig trees produce a latex protein that can cause cross-reactive hypersensitivity reactions in those allergic to F benjamina latex and rubber latex.⁶ The latex proteins in fig trees can act as airborne respiratory allergens. Ingestion of figs can produce anaphylactic reactions in those sensitized to rubber latex and F benjamina latex.⁷ Other plant families associated with phototoxic reactions include Rutaceae (lemon, lime, bitter orange), Apiaceae (formerly Umbelliferae)(carrot, parsnip, parsley, dill, celery, hogweed), and Fabaceae (prairie turnip).

Most cases of fig phytophotodermatitis begin with burning, pain, and/or itching within hours of sunlight exposure in areas of the skin that encountered components of the fig tree, often in a linear pattern. The affected areas become erythematous and edematous with formation of bullae and unilocular vesicles over the course of 1 to 3 days.^12,14,15 Lesions may extend beyond the region of contact with the fig tree as they spread across the skin due to sweat or friction, and pain may linger even after the lesions resolve.^12,13,16 Adults who handle fig trees (eg, pruning) are susceptible to phototoxic reactions, especially those using chain saws or other mechanisms that result in spray exposure, as the photosensitizing sap permeates the wood and bark of the entire tree.¹⁷ Similarly, children who handle fig leaves or sap during outdoor play can develop bullous eruptions. Severe cases have resulted in hospital admission after prolonged exposure.¹⁶ Additionally, irritant dermatitis may arise from contact with the trichomes or “hairs” on various parts of the plant.

Image provided with permission by Scott Norton, MD, MPH, MSc (Washington, DC).

Patients who use natural remedies containing components of the fig tree without the supervision of a medical provider put themselves at risk for unsafe or unwanted adverse effects, such as phytophotodermatitis.^12,15,16,18 An entire family presented with burns after they applied fig leaf extract to the skin prior to tanning outside in the sun.¹⁹ A 42-year-old woman acquired a severe burn covering 81% of the body surface after topically applying fig leaf tea to the skin as a tanning agent.²⁰ A subset of patients ingesting or applying fig tree components for conditions such as vitiligo, dermatitis, onychomycosis, and motor retardation developed similar cutaneous reactions.^13,14,21,22 Lesions resembling finger marks can raise concerns for potential abuse or neglect in children.²²

The differential diagnosis for fig phytophotodermatitis includes sunburn, chemical burns, drug-related photosensitivity, infectious lesions (eg, herpes simplex, bullous impetigo, Lyme disease, superficial lymphangitis), connective tissue disease (eg, systemic lupus erythematosus), contact dermatitis, and nonaccidental trauma.^12,15,18 Compared to sunburn, phytophotodermatitis tends to increase in severity over days following exposure and heals with dramatic hyperpigmentation, which also prompts visits to dermatology.¹²

Treatment

Treatment of fig phytophotodermatitis chiefly is symptomatic, including analgesia, appropriate wound care, and infection prophylaxis. Topical and systemic corticosteroids may aid in the resolution of moderate to severe reactions.^15,23,24 Even severe injuries over small areas or mild injuries to a high percentage of the total body surface area may require treatment in a burn unit. Patients should be encouraged to use mineral-based sunscreens on the affected areas to reduce the risk for hyperpigmentation. Individuals who regularly handle fig trees should use contact barriers including gloves and protective clothing (eg, long-sleeved shirts, long pants).

Plant Parts and Nomenclature

Ficus carica (common fig) is a deciduous shrub or small tree with smooth gray bark that can grow up to 10 m in height (Figure 1). It is characterized by many spreading branches, but the trunk rarely grows beyond a diameter of 7 in. Its hairy leaves are coarse on the upper side and soft underneath with 3 to 7 deep lobes that can extend up to 25 cm in length or width; the leaves grow individually, alternating along the sides of the branches. Fig trees often can be seen adorning yards, gardens, and parks, especially in tropical and subtropical climates. Ficus carica should not be confused with Ficus benjamina (weeping fig), a common ornamental tree that also is used to provide shade in hot climates, though both can cause phototoxic skin eruptions.

The common fig tree originated in the Mediterranean and western Asia¹ and has been cultivated by humans since the second and third millennia bc for its fruit, which commonly is used to sweeten cookies, cakes, and jams.² Figs are the most commonly mentioned food plant in the Bible, with at least 56 references in the Old and New Testaments.³ The “fruit” technically is a syconium—a hollow fleshy receptacle with a small opening at the apex partly closed by small scales. It can be obovoid, turbinate, or pear shaped; can be 1 to 4 inches long; and can vary in color from yellowish green to coppery, bronze, or dark purple (Figure 2).

Ficus carica is a member of the Moraceae family (derived from the Latin name for the mulberry tree), which includes 53 genera and approximately 1400 species, of which about 850 belong to the genus Ficus (the Latin name for a fig tree). The term carica likely comes from the Latin word carricare (to load) to describe a tree loaded with figs. Family members include trees, shrubs, lianas, and herbs that usually contain laticifers with a milky latex.

Traditional Uses

For centuries, components of the fig tree have been used in herbal teas and pastes to treat ailments ranging from sore throats to diarrhea, though there is no evidence to support their efficacy.⁴ Ancient Indians and Egyptians used plants such as the common fig tree containing furocoumarins to induce hyperpigmentation in vitiligo.⁵

Phototoxic Components

The leaves and sap of the common fig tree contain psoralens, which are members of the furocoumarin group of chemical compounds and are the source of its phototoxicity. The fruit does not contain psoralens.^6-9 The tree also produces proteolytic enzymes such as protease, amylase, ficin, triterpenoids, and lipodiastase that enhance its phototoxic effects.⁸ Exposure to UV light between 320 and 400 nm following contact with these phototoxic components triggers a reaction in the skin over the course of 1 to 3 days.⁵ The psoralens bind in epidermal cells, cross-link the DNA, and cause cell-membrane destruction, leading to edema and necrosis.¹⁰ The delay in symptoms may be attributed to the time needed to synthesize acute-phase reaction proteins such as tumor necrosis factor α and IL-1.¹¹ In spring and summer months, an increased concentration of psoralens in the leaves and sap contribute to an increased incidence of phytophotodermatitis.⁹ Humidity and sweat also increase the percutaneous absorption of psoralens.^12,13

Allergens

Fig trees produce a latex protein that can cause cross-reactive hypersensitivity reactions in those allergic to F benjamina latex and rubber latex.⁶ The latex proteins in fig trees can act as airborne respiratory allergens. Ingestion of figs can produce anaphylactic reactions in those sensitized to rubber latex and F benjamina latex.⁷ Other plant families associated with phototoxic reactions include Rutaceae (lemon, lime, bitter orange), Apiaceae (formerly Umbelliferae)(carrot, parsnip, parsley, dill, celery, hogweed), and Fabaceae (prairie turnip).

Most cases of fig phytophotodermatitis begin with burning, pain, and/or itching within hours of sunlight exposure in areas of the skin that encountered components of the fig tree, often in a linear pattern. The affected areas become erythematous and edematous with formation of bullae and unilocular vesicles over the course of 1 to 3 days.^12,14,15 Lesions may extend beyond the region of contact with the fig tree as they spread across the skin due to sweat or friction, and pain may linger even after the lesions resolve.^12,13,16 Adults who handle fig trees (eg, pruning) are susceptible to phototoxic reactions, especially those using chain saws or other mechanisms that result in spray exposure, as the photosensitizing sap permeates the wood and bark of the entire tree.¹⁷ Similarly, children who handle fig leaves or sap during outdoor play can develop bullous eruptions. Severe cases have resulted in hospital admission after prolonged exposure.¹⁶ Additionally, irritant dermatitis may arise from contact with the trichomes or “hairs” on various parts of the plant.

Image provided with permission by Scott Norton, MD, MPH, MSc (Washington, DC).

Patients who use natural remedies containing components of the fig tree without the supervision of a medical provider put themselves at risk for unsafe or unwanted adverse effects, such as phytophotodermatitis.^12,15,16,18 An entire family presented with burns after they applied fig leaf extract to the skin prior to tanning outside in the sun.¹⁹ A 42-year-old woman acquired a severe burn covering 81% of the body surface after topically applying fig leaf tea to the skin as a tanning agent.²⁰ A subset of patients ingesting or applying fig tree components for conditions such as vitiligo, dermatitis, onychomycosis, and motor retardation developed similar cutaneous reactions.^13,14,21,22 Lesions resembling finger marks can raise concerns for potential abuse or neglect in children.²²

The differential diagnosis for fig phytophotodermatitis includes sunburn, chemical burns, drug-related photosensitivity, infectious lesions (eg, herpes simplex, bullous impetigo, Lyme disease, superficial lymphangitis), connective tissue disease (eg, systemic lupus erythematosus), contact dermatitis, and nonaccidental trauma.^12,15,18 Compared to sunburn, phytophotodermatitis tends to increase in severity over days following exposure and heals with dramatic hyperpigmentation, which also prompts visits to dermatology.¹²

Treatment

Treatment of fig phytophotodermatitis chiefly is symptomatic, including analgesia, appropriate wound care, and infection prophylaxis. Topical and systemic corticosteroids may aid in the resolution of moderate to severe reactions.^15,23,24 Even severe injuries over small areas or mild injuries to a high percentage of the total body surface area may require treatment in a burn unit. Patients should be encouraged to use mineral-based sunscreens on the affected areas to reduce the risk for hyperpigmentation. Individuals who regularly handle fig trees should use contact barriers including gloves and protective clothing (eg, long-sleeved shirts, long pants).

In 2023, ESPEN (the European Society for Clinical Nutrition and Metabolism) published consensus recommendations highlighting the importance of regular monitoring and treatment of nutrient deficiencies in patients with inflammatory bowel disease (IBD) for improved prognosis, mortality, and quality of life.¹ Suboptimal nutrition in patients with IBD predominantly results from inflammation of the gastrointestinal (GI) tract leading to malabsorption; however, medications commonly used to manage IBD also can contribute to malnutrition.^2,3 Additionally, patients may develop nausea and food avoidance due to medication or the disease itself, leading to nutritional withdrawal and eventual deficiency.⁴ Even with the development of diets focused on balancing nutritional needs and decreasing inflammation,⁵ offsetting this aversion to food can be difficult to overcome.²

Cutaneous manifestations of IBD are multifaceted and can be secondary to the disease, reactive to or associated with IBD, or effects from nutritional deficiencies. The most common vitamin and nutrient deficiencies in patients with IBD include iron; zinc; calcium; vitamin D; and vitamins B₆ (pyridoxine), B₉ (folic acid), and B₁₂.⁶ Malnutrition may manifest with cutaneous disease, and dermatologists can be the first to identify and assess for nutritional deficiencies. In this article, we review the mechanisms of these micronutrient depletions in the context of IBD, their subsequent dermatologic manifestations (Table), and treatment and monitoring guidelines for each deficiency.

Iron

A systematic review conducted from 2007 to 2012 in European patients with IBD (N=2192) found the overall prevalence of anemia in this population to be 24% (95% CI, 18%-31%), with 57% of patients with anemia experiencing iron deficiency.⁷ Anemia is observed more commonly in patients hospitalized with IBD and is common in patients with both Crohn disease and ulcerative colitis.⁸

Pathophysiology—Iron is critically important in oxygen transportation throughout the body as a major component of hemoglobin. Physiologically, the low pH of the duodenum and proximal jejunum allows divalent metal transporter 1 to transfer dietary Fe³⁺ into enterocytes, where it is reduced to the transportable Fe²⁺.^9,10 Distribution of Fe²⁺ ions from enterocytes relies on ferroportin, an iron-transporting protein, which is heavily regulated by the protein hepcidin.¹¹ Hepcidin, a known acute phase reactant, will increase in the setting of active IBD, causing a depletion of ferroportin and an inability of the body to utilize the stored iron in enterocytes.¹² This poor utilization of iron stores combined with blood loss caused by inflammation in the GI tract is the proposed primary mechanism of iron-deficiency anemia observed in patients with IBD.¹³

Cutaneous Manifestations—From a dermatologic perspective, iron-deficiency anemia can manifest with a wide range of symptoms including glossitis, koilonychia, xerosis and/or pruritus, and brittle hair or hair loss.^14,15 Although the underlying pathophysiology of these cutaneous manifestations is not fully understood, there are several theories assessing the mechanisms behind the skin findings of iron deficiency.

Atrophic glossitis has been observed in many patients with iron deficiency and is thought to manifest due to low iron concentrations in the blood, thereby decreasing oxygen delivery to the papillae of the dorsal tongue with resultant atrophy.^16,17 Similarly, decreased oxygen delivery to the nail bed capillaries may cause deformities in the nail called koilonychia (or “spoon nails”).¹⁸ Iron is a key co-factor in collagen lysyl hydroxylase that promotes collagen binding; iron deficiency may lead to disruptions in the epidermal barrier that can cause pruritus and xerosis.¹⁹ An observational study of 200 healthy patients with a primary concern of pruritus found a correlation between low serum ferritin and a higher degree of pruritus (r=−0.768; P<.00001).²⁰

Evidence for iron’s role in hair growth comes from a mouse model study with a mutation in the serine protease TMPRSS6—a protein that regulates hepcidin and iron absorption—which caused an increase in hepcidin production and subsequent systemic iron deficiency. Mice at 4 weeks of age were devoid of all body hair but had substantial regrowth after initiation of a 2-week iron-rich diet, which suggests a connection between iron repletion and hair growth in mice with iron deficiency.²¹ Additionally, a meta-analysis analyzing the comorbidities of patients with alopecia areata found them to have higher odds (odds ratio [OR]=2.78; 95% CI, 1.23-6.29) of iron-deficiency anemia but no association with IBD (OR=1.48; 95% CI, 0.32-6.82).²²

Diagnosis and Monitoring—The American Gastroenterological Association recommends a complete blood cell count (CBC), serum ferritin, transferrin saturation (TfS), and C-reactive protein (CRP) as standard evaluations for iron deficiency in patients with IBD. Patients with active IBD should be screened every 3 months,and patients with inactive disease should be screened every 6 to 12 months.²³

Although ferritin and TfS often are used as markers for iron status in healthy individuals, they are positive and negative acute phase reactants, respectively. Using them to assess iron status in patients with IBD may inaccurately represent iron status in the setting of inflammation from the disease.²⁴ The European Crohn’s and Colitis Organisation (ECCO) produced guidelines to define iron deficiency as a TfS less than 20% or a ferritin level less than 30 µg/L in patients without evidence of active IBD and a ferritin level less than 100 µg/L for patients with active inflammation.²⁵

A 2020 multicenter observational study of 202 patients with diagnosed IBD found that the ECCO guideline of ferritin less than 30 µg/L had an area under the receiver operating characteristic (AUROC) curve of 0.69, a sensitivity of 0.43, and a specificity of 0.95 in their population.²⁶ In a sensitivity analysis stratifying patients by CRP level (<10 or ≥10 mg/L), the authors found that for patients with ulcerative colitis and a CRP less than 10 mg/L, a cut-off value of ferritin less than 65 µg/L (AUROC=0.78) had a sensitivity of 0.78 and specificity of 0.76, and a TfS value of less than 16% (AUROC=0.88) had a sensitivity of 0.79 and a specificity of 0.9. In patients with a CRP of 10 mg/L or greater, a cut-off value of ferritin 80 µg/L (AUROC=0.76) had a sensitivity of 0.75 and a specificity of 0.82, and a TfS value of less than 11% (AUROC=0.69) had a sensitivity of 0.79 and a specificity of 0.88. There were no ferritin cut-off values associated with good diagnostic performance (defined as both sensitivity and specificity >0.70) for iron deficiency in patients with Crohn disease.²⁶

The authors recommended using an alternative iron measurement such as soluble transferrin receptor (sTfR)/log ferritin ratio (TfR-F) that is not influenced by active inflammation and has a good correlation with ferritin values (TfR-F: r=0.66; P<.001).²⁶ However, both sTfR and TfR-F have high costs and intermethod variability as well as differences in their reference ranges depending on which laboratory performs the analysis, limiting the accessibility and practicality of easily obtaining these tests.²⁷ Although there may be inaccuracies for standard ferritin or TfS under ECCO guidelines, proposed alternatives have their own limitations, which may make ferritin and TfS the most reasonable evaluations of iron status as long as disease activity status at the time of testing is taken into consideration.

Treatment—Treatment of underlying iron deficiency in patients with IBD requires reversing the cause of the deficiency and supplementing iron. In patients with IBD, the options to supplement iron may be limited by active disease, making oral intake less effective. Oral iron supplementation also is associated with notable GI adverse effects that may be exacerbated in patients with IBD. A systematic review of 43 randomized controlled trials (RCTs) evaluating GI adverse effects (eg, nausea, abdominal pain, diarrhea, constipation, and black or tarry stools) of oral ferrous sulfate compared with placebo or intravenous (IV) iron supplementation in healthy nonanemic individuals found a significant increase in GI adverse effects with oral supplementation (placebo: OR=2.32; P<.0001; IV: OR=3.05; P<.0001).²⁸

Therefore, IV iron repletion may be necessary in patients with IBD and may require numerous infusions depending on the formulation of iron. In an RCT conducted in 2011, patients with iron-deficiency anemia with quiescent or mild to moderate IBD were treated with either IV iron sulfate or ferric carboxymaltose.²⁹ With a primary end point of hemoglobin response greater than 2 g/dL, the authors found that 150 of 240 patients responded to ferric carboxymaltose vs 118 of 235 treated with iron sulfate (P=.004). The dosing for ferric carboxymaltose was 1 to 3 infusions of 500 to 1000 mg of iron and for iron sulfate up to 11 infusions of 200 mg of iron.²⁹

Zinc

A systematic review of zinc deficiency in patients with IBD identified 7 studies including 2413 patients and revealed those with Crohn disease had a higher prevalence of zinc deficiency compared with patients with ulcerative colitis (54% vs 41%).³⁰

Pathophysiology—Zinc serves as a catalytic cofactor for enzymatic activity within proteins and immune cells.³¹ The homeostasis of zinc is tightly regulated within the brush border of the small intestine by zinc transporters ZIP4 and ZIP1 from the lumen of enterocytes into the bloodstream.³² Inflammation in the small intestine due to Crohn disease can result in zinc malabsorption.

Ranaldi et al³³ exposed intestinal cells and zinc-depleted intestinal cells to tumor necrosis factor α media to simulate an inflammatory environment. They measured transepithelial electrical resistance as a surrogate for transmembrane permeability and found that zinc-depleted cells had a statistically significantly higher transepithelial electrical resistance percentage (60% reduction after 4 hours; P<1.10^–6) when exposed to tumor necrosis factor α signaling compared with normal intestinal cells. They concluded that zinc deficiency can increase intestinal permeability in the presence of inflammation, creating a cycle of further nutrient malabsorption and inflammation exacerbating IBD symptoms.³³

Cutaneous Manifestations—After absorption in the small intestine, approximately 5% of zinc resides in the skin, with the highest concentration in the stratum spinosum.³⁴ A cell study found that keratinocytes in zinc-deficient environments had higher rates of apoptosis compared with cells in normal media. The authors proposed that this higher rate of apoptosis and the resulting inflammation could be a mechanism for developing the desquamative or eczematous scaly plaques that are common cutaneous manifestations of zinc deficiency.³⁵

Other cutaneous findings may include angular cheilitis, stomatitis, glossitis, paronychia, onychodystrophy, generalized alopecia, and delayed wound healing.³⁶ The histopathology of these skin lesions is characterized by granular layer loss, epidermal pallor, confluent parakeratosis, spongiosis, dyskeratosis, and psoriasiform hyperplasia.³⁷

Diagnosis and Monitoring—Assessing serum zinc levels is challenging, as they may decrease during states of inflammation.³⁸ A mouse model study showed a 3.1-fold increase (P<.001) in ZIP14 expression in wild-type mice compared with an IL-6 -/- knock-down model after IL-6 exposure. The authors concluded that the upregulation of ZIP14 in the liver due to inflammatory cytokine upregulation decreases zinc availability in serum.³⁹ Additionally, serum zinc can overestimate the level of deficiency in IBD because approximately 75% of serum zinc is bound to albumin, which decreases in the setting of inflammation.^40-42

Alternatively, alkaline phosphatase (AP), a zinc-dependent metalloenzyme, may be a better evaluator of zinc status during periods of inflammation. A study in rats evaluated zinc through serum zinc levels and AP levels after a period of induced stress to mimic a short-term inflammatory state.⁴³ The researchers found that total body stores of zinc were unaffected throughout the experiment; only serum zinc declined throughout the experiment duration while AP did not. Because approximately 75% of serum zinc is bound to serum albumin,⁴² the researchers concluded the induced inflammatory state depleted serum albumin and redistributed zinc to the liver, causing the observed serum zinc changes, while total body zinc levels and AP were largely unaffected in comparison.⁴³ Comorbid conditions such as liver or bone disease can increase AP levels, which limits the utility of AP as a surrogate for zinc in patients with comorbidities.⁴⁴ However, even in the context of active IBD, serum zinc still is currently considered the best biomarker to evaluate zinc status.⁴⁵

Treatment—The recommended dose for zinc supplementation is 20 to 40 mg daily with higher doses (>50 mg/d) for patients with malabsorptive syndromes such as IBD.⁴⁶ It can be administered orally or parenterally. Although rare, zinc replacement therapy may be associated with diarrhea, nausea, vomiting, mild headaches, and fatigue.⁴⁶ Additional considerations should be taken when repleting other micronutrients with zinc, as calcium and folate can inhibit zinc reabsorption, while zinc itself can inhibit iron and copper reabsorption.⁴⁷

Vitamin D and Calcium

Low vitamin D levels (<50 nmol/L) and hypocalcemia (<8.8 mg/dL) are common in patients with IBD.^48,49

Pathophysiology—Vitamin D levels are maintained via 2 mechanisms. The first mechanism is through the skin, as keratinocytes produce 7-dehydrocholesterol after exposure to UV light, which is converted into previtamin D₃ and then thermally isomerizes into vitamin D₃. This vitamin D₃ is then transported to the liver on vitamin D–binding protein.⁵⁰ The second mechanism is through oral vitamin D₃ that is absorbed through vitamin D receptors in intestinal epithelium and transported to the liver, where it is hydroxylated into 25-hydroxyvitamin D (25[OH]D), then to the kidneys for hydroxylation to 1,25(OH)₂D for redistribution throughout the body.⁵⁰ This activated form of vitamin D regulates calcium absorption in the intestine, and optimal vitamin D levels are necessary to absorb calcium efficiently.⁵¹ Inflammation from IBD within the small intestine can downregulate vitamin D receptors, causing malabsorption and decreased serum vitamin D.⁵²

Vitamin D signaling also is vital to maintaining the tight junctions and adherens junctions of the intestinal epithelium. Weakening the permeability of the epithelium further exacerbates malabsorption and subsequent vitamin D deficiency.⁵² A meta-analysis of 27 studies including 8316 patients with IBD showed low vitamin D levels were associated with increased odds of disease activity (OR=1.53; 95% CI, 1.32-1.77), mucosal inflammation (OR=1.25; 95% CI, 1.06-1.47), and future clinical relapse (OR=1.23; 95% CI, 1.03-1.47) in patients with Crohn disease. The authors concluded that low levels of vitamin D could be used as a potential biomarker of inflammatory status in Crohn disease.⁵³

Vitamin D and calcium are further implicated in maintaining skeletal health,⁴⁷ while vitamin D specifically helps maintain intestinal homeostasis⁵⁴ and immune system modulation in the skin.⁵⁵

Cutaneous Manifestations—Vitamin D is thought to play crucial roles in skin differentiation and proliferation, cutaneous innate immunity, hair follicle cycling, photoprotection, and wound healing.⁵⁶ Vitamin D deficiency has been observed in a large range of cutaneous diseases including skin cancer, psoriasis, vitiligo, bullous pemphigoid, atopic dermatitis, and various types of alopecia.^56-59 It is unclear whether vitamin D deficiency facilitates these disease processes or is merely the consequence of a disrupted cutaneous surface with the inability to complete the first step in vitamin D processing. A 2014 meta-analysis of 290 prospective cohort studies and 172 randomized trials concluded that 25(OH)D deficiency was associated with ill health and did not find causal evidence for any specific disease, dermatologic or otherwise.⁶⁰ Calcium deficiency may cause epidermal changes including dry skin, coarse hair, and brittle nails.⁶¹

Diagnosis and Monitoring—The ECCO guidelines recommend obtaining serum 25(OH)D levels every 3 months in patients with IBD.⁶² Levels less than 75 nmol/L are considered deficient, and a value less than 30 nmol/L increases the risk for osteomalacia and nutritional rickets, constituting severe vitamin D deficiency.^63-65

An observational study of 325 patients with IBD showed a statistically significant negative correlation between serum vitamin D and fecal calprotectin (r=−0.19; P<.001), a stool-based marker for gut inflammation, supporting vitamin D as a potential biomarker in IBD.⁶⁶

Evaluation of calcium can be done through serum levels in patients with IBD.⁶⁷ Patients with IBD are at risk for hypoalbuminemia; therefore, consideration should be taken to ensure calcium levels are corrected, as approximately 50% of calcium is bound to albumin or other ions in the body,⁶⁸ which can be done by adjusting the calcium concentration by 0.02 mmol/L for every 1 g/L of albumin above or below 40 g/L. In the most critically ill patients, a direct ionized calcium blood level should be used instead because the previously mentioned correction calculations are inaccurate when albumin is critically low.⁶⁹

Treatment—The ECCO guidelines recommend calcium and vitamin D repletion of 500 to 1000 mg and 800 to 1000 U, respectively, in patients with IBD on systemic corticosteroids to prevent the negative effects of bone loss.⁶² Calcium repletion in patients with IBD who are not on systemic steroids are the same as for the general population.⁶⁵

Vitamin D repletion also may help decrease IBD activity. In a prospective study, 10,000 IU/d of vitamin D in 10 patients with IBD—adjusted over 12 weeks to a target of 100 to 125 nmol/L of serum 25(OH)D—showed a significant reduction in clinical Crohn activity (P=.019) over the study period.⁷⁰ In contrast, 2000 IU/d for 3 months in an RCT of 27 patients with Crohn disease found significantly lower CRP (P=.019) and significantly higher self-reported quality of life (P=.037) but nonsignificant decreases in Crohn activity (P=.082) in patients with 25(OH)D levels of 75 nmol/L or higher compared with those with 25(OH)D levels less than 75 nmol/L.⁷¹

These discrepancies illustrate the need for expanded clinical trials to elucidate the optimal vitamin D dosing for patients with IBD. Ultimately, assessing vitamin D and calcium status and considering repletion in patients with IBD, especially those with comorbid dermatologic diseases such as poor wound healing, psoriasis, or atopic dermatitis, is important.

Vitamin B₆ (Pyridoxine)

Pathophysiology—Pyridoxine is an important coenzyme for many functions including amino acid transamination, fatty acid metabolism, and conversion of tryptophan to niacin. It is absorbed in the jejunum and ileum and subsequently transported to the liver for rephosphorylation and release into its active form.³⁶ An observational study assessing the nutritional status of patients with IBD found that only 5.7% of 105 patients with food records had inadequate dietary intake of pyridoxine, but 29% of all patients with IBD had subnormal pyridoxine levels.⁷² Additionally, they found no significant difference in the prevalence of subnormal pyridoxine levels in patients with active IBD vs IBD in remission. The authors suggested that the subnormal pyridoxine levels in patients with IBD likely were multifactorial and resulted from malabsorption due to active disease, inflammation, and inadequate intake.⁷²

Cutaneous Manifestations—Cutaneous findings associated with pyridoxine deficiency include periorificial and perineal dermatitis,⁷³ angular stomatitis, and cheilitis with associated burning, redness, and tongue edema.³⁶ Additionally, pyridoxine is involved in the conversion of tryptophan to niacin, and its deficiency may manifest with pellagralike findings.⁷⁴

Because pyridoxine is critical to protein metabolism, its deficiency may disrupt key cellular structures that rely on protein concentrations to maintain structural integrity. One such structure in the skin that heavily relies on protein concentrations is the ground substance of the extracellular matrix—the amorphous gelatinous spaces that occupy the areas between the extracellular matrix, which consists of cross-linked glycosaminoglycans and proteins.⁷⁵ Without protein, ground substance increases in viscosity and can disrupt the epidermal barrier, leading to increased transepidermal water loss and ultimately inflammation.⁷⁶ Although this theory has yet to be validated fully, this is a potential mechanistic explanation for the inflammation in dermal papillae that leads to dermatitis observed in pyridoxine deficiency.

Diagnosis and Monitoring—Direct biomarkers of pyridoxine status are in serum, plasma, erythrocytes, and urine, with the most common measurement in plasma as pyridoxal 5′-phosphate (PLP).⁷⁷ Plasma PLP concentrations lower than 20 nmol/L are suggestive of deficiency.⁷⁸ Plasma PLP has shown inverse relationships with acute phase inflammatory markers CRP⁷⁹ and AP,⁷⁸ thereby raising concerns for its validity to assess pyridoxine status in patients with symptomatic IBD.⁸⁰

Alternative evaluations of pyridoxine include tryptophan and methionine loading tests,³⁶ which are measured via urinary excretion and require normal kidney function to be accurate. They should be considered in IBD if necessary, but routine testing, even in patients with symptomatic IBD, is not recommended in the ECCO guidelines. Additional considerations should be taken in patients with altered nutrient requirements such as those who have undergone bowel resection due to highly active disease or those who receive parenteral nutritional supplementation.⁸¹

Treatment—Recommendations for oral pyridoxine supplementation range from 25 to 600 mg daily,⁸² with symptoms typically improving on 100 mg daily.³⁶ Pyridoxine supplementation may have additional benefits for patients with IBD and potentially modulate disease severity. An IL-10 knockout mouse supplemented with pyridoxine had an approximately 60% reduction (P<.05) in inflammation compared to mice deficient in pyridoxine.⁸³ The authors suggest that PLP-dependent enzymes can inhibit further proinflammatory signaling and T-cell migration that can exacerbate IBD. Ultimately, more data is needed before determining the efficacy of pyridoxine supplementation for active IBD.

Vitamin B₁₂ and Vitamin B₉ (Folic Acid)

Pathophysiology—Vitamin B₁₂ is reabsorbed in the terminal ileum, the distal portion of the small intestine. The American Gastroenterological Association recommends that patients with a history of extensive ileal disease or prior ileal surgery, which is the case for many patients with Crohn disease, be monitored for vitamin B₁₂ deficiency.²³ Monitoring and rapid supplementation of vitamin B₁₂ can prevent pernicious anemia and irreversible neurologic damage that may result from deficiency.⁸⁴

Folic acid is primarily absorbed in the duodenum and jejunum of the small intestine. A meta-analysis performed in 2017 assessed studies observing folic acid and vitamin B₁₂ levels in 1086 patients with IBD compared with 1484 healthy controls and found an average difference in serum folate concentration of 0.46 nmol/L (P<.001).⁸⁴ Interestingly, this study did not find a significant difference in serum vitamin B₁₂ levels between patients with IBD and healthy controls, highlighting the mechanism of vitamin B₁₂ deficiency in IBD because only patients with terminal ileal involvement are at risk for malabsorption and subsequent deficiency.

Cutaneous Manifestations—Both vitamin B₁₂ and folic acid deficiency can manifest as cheilitis, glossitis, and/or generalized hyperpigmentation that is accentuated in the flexural areas, palms, soles, and oral cavity.^85,86 Systemic symptoms of patients with vitamin B₁₂ and folic acid deficiency include megaloblastic anemia, pallor, and fatigue. A potential mechanism for the hyperpigmentation observed from vitamin B₁₂ deficiency came from an electron microscope study that showed an increased concentration of melanosomes in a patient with deficiency.⁸⁷

Diagnosis and Monitoring—In patients with suspected vitamin B₁₂ and/or folic acid deficiency, initial evaluation should include a CBC with peripheral smear and serum vitamin B₁₂ and folate levels. In cases for which the diagnosis still is unclear after initial testing, methylmalonic acid and homocysteine levels can help differentiate between the 2 deficiencies. Methylmalonic acid classically is elevated (>260 nmol/L) in vitamin B₁₂ deficiency but not in folate deficiency.⁸⁸ Cut-off values for vitamin B₁₂ deficiency are less than 200 to 250 pg/mL forserum vitamin B₁₂ and/or an elevated level of methylmalonic acid (>0.271 µmol/L).⁸⁹ A serum folic acid value greater than 3 ng/mL and/or erythrocyte folate concentrations greater than 140 ng/mL are considered adequate, whereas an indicator of folic acid deficiency is a homocysteine level less than 10 µmol/L.⁹⁰ A CBC can screen for macrocytic megaloblastic anemias (mean corpuscular volume >100 fl), which are classic diagnostic signs of an underlying vitamin B₁₂ or folate deficiency.

Treatment—According to the Centers for Disease Control and Prevention, supplementation of vitamin B₁₂ can be done orally with 1000 µg daily in patients with deficiency. In patients with active IBD, oral reabsorption of vitamin B₁₂ can be less effective, making subcutaneous or intramuscular administration (1000 µg/wk for 8 weeks, then monthly for life) better options.⁸⁹

Patients with IBD managed with methotrexate should be screened carefully for folate deficiency. Methotrexate is a folate analog that sometimes is used for the treatment of IBD. Reversible competitive inhibition of dihydrofolate reductase can precipitate a systemic folic acid decrease.⁹¹ Typically, oral folic acid (1 to 5 mg/d) is sufficient to treat folate deficiency, with the ESPEN recommending 5 mg once weekly 24 to 72 hours after methotrexate treatment or 1 mg daily for 5 days per week in patients with IBD.¹ Alternative formulations—IV, subcutaneous, or intramuscular—are available for patients who cannot tolerate oral intake.⁹²

Final Thoughts

Dermatologists can be the first to observe the cutaneous manifestations of micronutrient deficiencies. Although the symptoms of each micronutrient deficiency discussed may overlap, attention to small clinical clues in patients with IBD can improve patient outcomes and quality of life. For example, koilonychia with glossitis and xerosis likely is due to iron deficiency, while zinc deficiency should be suspected in patients with scaly eczematous plaques in skin folds. A high level of suspicion for micronutrient deficiencies in patients with IBD should be followed by a complete patient history, review of systems, and thorough clinical examination. A thorough laboratory evaluation can pinpoint nutritional deficiencies in patients with IBD, keeping in mind that specific biomarkers such as ferritin and serum zinc also act as acute phase reactants and should be interpreted in this context. Co-management with gastroenterologists should be a priority in patients with IBD, as gaining control of inflammatory disease is crucial for the prevention of recurrent vitamin and micronutrient deficiencies in addition to long-term health in this population.

In 2023, ESPEN (the European Society for Clinical Nutrition and Metabolism) published consensus recommendations highlighting the importance of regular monitoring and treatment of nutrient deficiencies in patients with inflammatory bowel disease (IBD) for improved prognosis, mortality, and quality of life.¹ Suboptimal nutrition in patients with IBD predominantly results from inflammation of the gastrointestinal (GI) tract leading to malabsorption; however, medications commonly used to manage IBD also can contribute to malnutrition.^2,3 Additionally, patients may develop nausea and food avoidance due to medication or the disease itself, leading to nutritional withdrawal and eventual deficiency.⁴ Even with the development of diets focused on balancing nutritional needs and decreasing inflammation,⁵ offsetting this aversion to food can be difficult to overcome.²

Cutaneous manifestations of IBD are multifaceted and can be secondary to the disease, reactive to or associated with IBD, or effects from nutritional deficiencies. The most common vitamin and nutrient deficiencies in patients with IBD include iron; zinc; calcium; vitamin D; and vitamins B₆ (pyridoxine), B₉ (folic acid), and B₁₂.⁶ Malnutrition may manifest with cutaneous disease, and dermatologists can be the first to identify and assess for nutritional deficiencies. In this article, we review the mechanisms of these micronutrient depletions in the context of IBD, their subsequent dermatologic manifestations (Table), and treatment and monitoring guidelines for each deficiency.

Iron

A systematic review conducted from 2007 to 2012 in European patients with IBD (N=2192) found the overall prevalence of anemia in this population to be 24% (95% CI, 18%-31%), with 57% of patients with anemia experiencing iron deficiency.⁷ Anemia is observed more commonly in patients hospitalized with IBD and is common in patients with both Crohn disease and ulcerative colitis.⁸

Pathophysiology—Iron is critically important in oxygen transportation throughout the body as a major component of hemoglobin. Physiologically, the low pH of the duodenum and proximal jejunum allows divalent metal transporter 1 to transfer dietary Fe³⁺ into enterocytes, where it is reduced to the transportable Fe²⁺.^9,10 Distribution of Fe²⁺ ions from enterocytes relies on ferroportin, an iron-transporting protein, which is heavily regulated by the protein hepcidin.¹¹ Hepcidin, a known acute phase reactant, will increase in the setting of active IBD, causing a depletion of ferroportin and an inability of the body to utilize the stored iron in enterocytes.¹² This poor utilization of iron stores combined with blood loss caused by inflammation in the GI tract is the proposed primary mechanism of iron-deficiency anemia observed in patients with IBD.¹³

Cutaneous Manifestations—From a dermatologic perspective, iron-deficiency anemia can manifest with a wide range of symptoms including glossitis, koilonychia, xerosis and/or pruritus, and brittle hair or hair loss.^14,15 Although the underlying pathophysiology of these cutaneous manifestations is not fully understood, there are several theories assessing the mechanisms behind the skin findings of iron deficiency.

Atrophic glossitis has been observed in many patients with iron deficiency and is thought to manifest due to low iron concentrations in the blood, thereby decreasing oxygen delivery to the papillae of the dorsal tongue with resultant atrophy.^16,17 Similarly, decreased oxygen delivery to the nail bed capillaries may cause deformities in the nail called koilonychia (or “spoon nails”).¹⁸ Iron is a key co-factor in collagen lysyl hydroxylase that promotes collagen binding; iron deficiency may lead to disruptions in the epidermal barrier that can cause pruritus and xerosis.¹⁹ An observational study of 200 healthy patients with a primary concern of pruritus found a correlation between low serum ferritin and a higher degree of pruritus (r=−0.768; P<.00001).²⁰

Evidence for iron’s role in hair growth comes from a mouse model study with a mutation in the serine protease TMPRSS6—a protein that regulates hepcidin and iron absorption—which caused an increase in hepcidin production and subsequent systemic iron deficiency. Mice at 4 weeks of age were devoid of all body hair but had substantial regrowth after initiation of a 2-week iron-rich diet, which suggests a connection between iron repletion and hair growth in mice with iron deficiency.²¹ Additionally, a meta-analysis analyzing the comorbidities of patients with alopecia areata found them to have higher odds (odds ratio [OR]=2.78; 95% CI, 1.23-6.29) of iron-deficiency anemia but no association with IBD (OR=1.48; 95% CI, 0.32-6.82).²²

Diagnosis and Monitoring—The American Gastroenterological Association recommends a complete blood cell count (CBC), serum ferritin, transferrin saturation (TfS), and C-reactive protein (CRP) as standard evaluations for iron deficiency in patients with IBD. Patients with active IBD should be screened every 3 months,and patients with inactive disease should be screened every 6 to 12 months.²³

Although ferritin and TfS often are used as markers for iron status in healthy individuals, they are positive and negative acute phase reactants, respectively. Using them to assess iron status in patients with IBD may inaccurately represent iron status in the setting of inflammation from the disease.²⁴ The European Crohn’s and Colitis Organisation (ECCO) produced guidelines to define iron deficiency as a TfS less than 20% or a ferritin level less than 30 µg/L in patients without evidence of active IBD and a ferritin level less than 100 µg/L for patients with active inflammation.²⁵

A 2020 multicenter observational study of 202 patients with diagnosed IBD found that the ECCO guideline of ferritin less than 30 µg/L had an area under the receiver operating characteristic (AUROC) curve of 0.69, a sensitivity of 0.43, and a specificity of 0.95 in their population.²⁶ In a sensitivity analysis stratifying patients by CRP level (<10 or ≥10 mg/L), the authors found that for patients with ulcerative colitis and a CRP less than 10 mg/L, a cut-off value of ferritin less than 65 µg/L (AUROC=0.78) had a sensitivity of 0.78 and specificity of 0.76, and a TfS value of less than 16% (AUROC=0.88) had a sensitivity of 0.79 and a specificity of 0.9. In patients with a CRP of 10 mg/L or greater, a cut-off value of ferritin 80 µg/L (AUROC=0.76) had a sensitivity of 0.75 and a specificity of 0.82, and a TfS value of less than 11% (AUROC=0.69) had a sensitivity of 0.79 and a specificity of 0.88. There were no ferritin cut-off values associated with good diagnostic performance (defined as both sensitivity and specificity >0.70) for iron deficiency in patients with Crohn disease.²⁶

The authors recommended using an alternative iron measurement such as soluble transferrin receptor (sTfR)/log ferritin ratio (TfR-F) that is not influenced by active inflammation and has a good correlation with ferritin values (TfR-F: r=0.66; P<.001).²⁶ However, both sTfR and TfR-F have high costs and intermethod variability as well as differences in their reference ranges depending on which laboratory performs the analysis, limiting the accessibility and practicality of easily obtaining these tests.²⁷ Although there may be inaccuracies for standard ferritin or TfS under ECCO guidelines, proposed alternatives have their own limitations, which may make ferritin and TfS the most reasonable evaluations of iron status as long as disease activity status at the time of testing is taken into consideration.

Treatment—Treatment of underlying iron deficiency in patients with IBD requires reversing the cause of the deficiency and supplementing iron. In patients with IBD, the options to supplement iron may be limited by active disease, making oral intake less effective. Oral iron supplementation also is associated with notable GI adverse effects that may be exacerbated in patients with IBD. A systematic review of 43 randomized controlled trials (RCTs) evaluating GI adverse effects (eg, nausea, abdominal pain, diarrhea, constipation, and black or tarry stools) of oral ferrous sulfate compared with placebo or intravenous (IV) iron supplementation in healthy nonanemic individuals found a significant increase in GI adverse effects with oral supplementation (placebo: OR=2.32; P<.0001; IV: OR=3.05; P<.0001).²⁸

Therefore, IV iron repletion may be necessary in patients with IBD and may require numerous infusions depending on the formulation of iron. In an RCT conducted in 2011, patients with iron-deficiency anemia with quiescent or mild to moderate IBD were treated with either IV iron sulfate or ferric carboxymaltose.²⁹ With a primary end point of hemoglobin response greater than 2 g/dL, the authors found that 150 of 240 patients responded to ferric carboxymaltose vs 118 of 235 treated with iron sulfate (P=.004). The dosing for ferric carboxymaltose was 1 to 3 infusions of 500 to 1000 mg of iron and for iron sulfate up to 11 infusions of 200 mg of iron.²⁹

Zinc

A systematic review of zinc deficiency in patients with IBD identified 7 studies including 2413 patients and revealed those with Crohn disease had a higher prevalence of zinc deficiency compared with patients with ulcerative colitis (54% vs 41%).³⁰

Pathophysiology—Zinc serves as a catalytic cofactor for enzymatic activity within proteins and immune cells.³¹ The homeostasis of zinc is tightly regulated within the brush border of the small intestine by zinc transporters ZIP4 and ZIP1 from the lumen of enterocytes into the bloodstream.³² Inflammation in the small intestine due to Crohn disease can result in zinc malabsorption.

Ranaldi et al³³ exposed intestinal cells and zinc-depleted intestinal cells to tumor necrosis factor α media to simulate an inflammatory environment. They measured transepithelial electrical resistance as a surrogate for transmembrane permeability and found that zinc-depleted cells had a statistically significantly higher transepithelial electrical resistance percentage (60% reduction after 4 hours; P<1.10^–6) when exposed to tumor necrosis factor α signaling compared with normal intestinal cells. They concluded that zinc deficiency can increase intestinal permeability in the presence of inflammation, creating a cycle of further nutrient malabsorption and inflammation exacerbating IBD symptoms.³³

Cutaneous Manifestations—After absorption in the small intestine, approximately 5% of zinc resides in the skin, with the highest concentration in the stratum spinosum.³⁴ A cell study found that keratinocytes in zinc-deficient environments had higher rates of apoptosis compared with cells in normal media. The authors proposed that this higher rate of apoptosis and the resulting inflammation could be a mechanism for developing the desquamative or eczematous scaly plaques that are common cutaneous manifestations of zinc deficiency.³⁵

Other cutaneous findings may include angular cheilitis, stomatitis, glossitis, paronychia, onychodystrophy, generalized alopecia, and delayed wound healing.³⁶ The histopathology of these skin lesions is characterized by granular layer loss, epidermal pallor, confluent parakeratosis, spongiosis, dyskeratosis, and psoriasiform hyperplasia.³⁷

Diagnosis and Monitoring—Assessing serum zinc levels is challenging, as they may decrease during states of inflammation.³⁸ A mouse model study showed a 3.1-fold increase (P<.001) in ZIP14 expression in wild-type mice compared with an IL-6 -/- knock-down model after IL-6 exposure. The authors concluded that the upregulation of ZIP14 in the liver due to inflammatory cytokine upregulation decreases zinc availability in serum.³⁹ Additionally, serum zinc can overestimate the level of deficiency in IBD because approximately 75% of serum zinc is bound to albumin, which decreases in the setting of inflammation.^40-42

Alternatively, alkaline phosphatase (AP), a zinc-dependent metalloenzyme, may be a better evaluator of zinc status during periods of inflammation. A study in rats evaluated zinc through serum zinc levels and AP levels after a period of induced stress to mimic a short-term inflammatory state.⁴³ The researchers found that total body stores of zinc were unaffected throughout the experiment; only serum zinc declined throughout the experiment duration while AP did not. Because approximately 75% of serum zinc is bound to serum albumin,⁴² the researchers concluded the induced inflammatory state depleted serum albumin and redistributed zinc to the liver, causing the observed serum zinc changes, while total body zinc levels and AP were largely unaffected in comparison.⁴³ Comorbid conditions such as liver or bone disease can increase AP levels, which limits the utility of AP as a surrogate for zinc in patients with comorbidities.⁴⁴ However, even in the context of active IBD, serum zinc still is currently considered the best biomarker to evaluate zinc status.⁴⁵

Treatment—The recommended dose for zinc supplementation is 20 to 40 mg daily with higher doses (>50 mg/d) for patients with malabsorptive syndromes such as IBD.⁴⁶ It can be administered orally or parenterally. Although rare, zinc replacement therapy may be associated with diarrhea, nausea, vomiting, mild headaches, and fatigue.⁴⁶ Additional considerations should be taken when repleting other micronutrients with zinc, as calcium and folate can inhibit zinc reabsorption, while zinc itself can inhibit iron and copper reabsorption.⁴⁷

Vitamin D and Calcium

Low vitamin D levels (<50 nmol/L) and hypocalcemia (<8.8 mg/dL) are common in patients with IBD.^48,49

Pathophysiology—Vitamin D levels are maintained via 2 mechanisms. The first mechanism is through the skin, as keratinocytes produce 7-dehydrocholesterol after exposure to UV light, which is converted into previtamin D₃ and then thermally isomerizes into vitamin D₃. This vitamin D₃ is then transported to the liver on vitamin D–binding protein.⁵⁰ The second mechanism is through oral vitamin D₃ that is absorbed through vitamin D receptors in intestinal epithelium and transported to the liver, where it is hydroxylated into 25-hydroxyvitamin D (25[OH]D), then to the kidneys for hydroxylation to 1,25(OH)₂D for redistribution throughout the body.⁵⁰ This activated form of vitamin D regulates calcium absorption in the intestine, and optimal vitamin D levels are necessary to absorb calcium efficiently.⁵¹ Inflammation from IBD within the small intestine can downregulate vitamin D receptors, causing malabsorption and decreased serum vitamin D.⁵²

Vitamin D signaling also is vital to maintaining the tight junctions and adherens junctions of the intestinal epithelium. Weakening the permeability of the epithelium further exacerbates malabsorption and subsequent vitamin D deficiency.⁵² A meta-analysis of 27 studies including 8316 patients with IBD showed low vitamin D levels were associated with increased odds of disease activity (OR=1.53; 95% CI, 1.32-1.77), mucosal inflammation (OR=1.25; 95% CI, 1.06-1.47), and future clinical relapse (OR=1.23; 95% CI, 1.03-1.47) in patients with Crohn disease. The authors concluded that low levels of vitamin D could be used as a potential biomarker of inflammatory status in Crohn disease.⁵³

Vitamin D and calcium are further implicated in maintaining skeletal health,⁴⁷ while vitamin D specifically helps maintain intestinal homeostasis⁵⁴ and immune system modulation in the skin.⁵⁵

Cutaneous Manifestations—Vitamin D is thought to play crucial roles in skin differentiation and proliferation, cutaneous innate immunity, hair follicle cycling, photoprotection, and wound healing.⁵⁶ Vitamin D deficiency has been observed in a large range of cutaneous diseases including skin cancer, psoriasis, vitiligo, bullous pemphigoid, atopic dermatitis, and various types of alopecia.^56-59 It is unclear whether vitamin D deficiency facilitates these disease processes or is merely the consequence of a disrupted cutaneous surface with the inability to complete the first step in vitamin D processing. A 2014 meta-analysis of 290 prospective cohort studies and 172 randomized trials concluded that 25(OH)D deficiency was associated with ill health and did not find causal evidence for any specific disease, dermatologic or otherwise.⁶⁰ Calcium deficiency may cause epidermal changes including dry skin, coarse hair, and brittle nails.⁶¹

Diagnosis and Monitoring—The ECCO guidelines recommend obtaining serum 25(OH)D levels every 3 months in patients with IBD.⁶² Levels less than 75 nmol/L are considered deficient, and a value less than 30 nmol/L increases the risk for osteomalacia and nutritional rickets, constituting severe vitamin D deficiency.^63-65

An observational study of 325 patients with IBD showed a statistically significant negative correlation between serum vitamin D and fecal calprotectin (r=−0.19; P<.001), a stool-based marker for gut inflammation, supporting vitamin D as a potential biomarker in IBD.⁶⁶

Evaluation of calcium can be done through serum levels in patients with IBD.⁶⁷ Patients with IBD are at risk for hypoalbuminemia; therefore, consideration should be taken to ensure calcium levels are corrected, as approximately 50% of calcium is bound to albumin or other ions in the body,⁶⁸ which can be done by adjusting the calcium concentration by 0.02 mmol/L for every 1 g/L of albumin above or below 40 g/L. In the most critically ill patients, a direct ionized calcium blood level should be used instead because the previously mentioned correction calculations are inaccurate when albumin is critically low.⁶⁹

Treatment—The ECCO guidelines recommend calcium and vitamin D repletion of 500 to 1000 mg and 800 to 1000 U, respectively, in patients with IBD on systemic corticosteroids to prevent the negative effects of bone loss.⁶² Calcium repletion in patients with IBD who are not on systemic steroids are the same as for the general population.⁶⁵

Vitamin D repletion also may help decrease IBD activity. In a prospective study, 10,000 IU/d of vitamin D in 10 patients with IBD—adjusted over 12 weeks to a target of 100 to 125 nmol/L of serum 25(OH)D—showed a significant reduction in clinical Crohn activity (P=.019) over the study period.⁷⁰ In contrast, 2000 IU/d for 3 months in an RCT of 27 patients with Crohn disease found significantly lower CRP (P=.019) and significantly higher self-reported quality of life (P=.037) but nonsignificant decreases in Crohn activity (P=.082) in patients with 25(OH)D levels of 75 nmol/L or higher compared with those with 25(OH)D levels less than 75 nmol/L.⁷¹

These discrepancies illustrate the need for expanded clinical trials to elucidate the optimal vitamin D dosing for patients with IBD. Ultimately, assessing vitamin D and calcium status and considering repletion in patients with IBD, especially those with comorbid dermatologic diseases such as poor wound healing, psoriasis, or atopic dermatitis, is important.

Vitamin B₆ (Pyridoxine)

Pathophysiology—Pyridoxine is an important coenzyme for many functions including amino acid transamination, fatty acid metabolism, and conversion of tryptophan to niacin. It is absorbed in the jejunum and ileum and subsequently transported to the liver for rephosphorylation and release into its active form.³⁶ An observational study assessing the nutritional status of patients with IBD found that only 5.7% of 105 patients with food records had inadequate dietary intake of pyridoxine, but 29% of all patients with IBD had subnormal pyridoxine levels.⁷² Additionally, they found no significant difference in the prevalence of subnormal pyridoxine levels in patients with active IBD vs IBD in remission. The authors suggested that the subnormal pyridoxine levels in patients with IBD likely were multifactorial and resulted from malabsorption due to active disease, inflammation, and inadequate intake.⁷²

Cutaneous Manifestations—Cutaneous findings associated with pyridoxine deficiency include periorificial and perineal dermatitis,⁷³ angular stomatitis, and cheilitis with associated burning, redness, and tongue edema.³⁶ Additionally, pyridoxine is involved in the conversion of tryptophan to niacin, and its deficiency may manifest with pellagralike findings.⁷⁴

Because pyridoxine is critical to protein metabolism, its deficiency may disrupt key cellular structures that rely on protein concentrations to maintain structural integrity. One such structure in the skin that heavily relies on protein concentrations is the ground substance of the extracellular matrix—the amorphous gelatinous spaces that occupy the areas between the extracellular matrix, which consists of cross-linked glycosaminoglycans and proteins.⁷⁵ Without protein, ground substance increases in viscosity and can disrupt the epidermal barrier, leading to increased transepidermal water loss and ultimately inflammation.⁷⁶ Although this theory has yet to be validated fully, this is a potential mechanistic explanation for the inflammation in dermal papillae that leads to dermatitis observed in pyridoxine deficiency.

Diagnosis and Monitoring—Direct biomarkers of pyridoxine status are in serum, plasma, erythrocytes, and urine, with the most common measurement in plasma as pyridoxal 5′-phosphate (PLP).⁷⁷ Plasma PLP concentrations lower than 20 nmol/L are suggestive of deficiency.⁷⁸ Plasma PLP has shown inverse relationships with acute phase inflammatory markers CRP⁷⁹ and AP,⁷⁸ thereby raising concerns for its validity to assess pyridoxine status in patients with symptomatic IBD.⁸⁰

Alternative evaluations of pyridoxine include tryptophan and methionine loading tests,³⁶ which are measured via urinary excretion and require normal kidney function to be accurate. They should be considered in IBD if necessary, but routine testing, even in patients with symptomatic IBD, is not recommended in the ECCO guidelines. Additional considerations should be taken in patients with altered nutrient requirements such as those who have undergone bowel resection due to highly active disease or those who receive parenteral nutritional supplementation.⁸¹

Treatment—Recommendations for oral pyridoxine supplementation range from 25 to 600 mg daily,⁸² with symptoms typically improving on 100 mg daily.³⁶ Pyridoxine supplementation may have additional benefits for patients with IBD and potentially modulate disease severity. An IL-10 knockout mouse supplemented with pyridoxine had an approximately 60% reduction (P<.05) in inflammation compared to mice deficient in pyridoxine.⁸³ The authors suggest that PLP-dependent enzymes can inhibit further proinflammatory signaling and T-cell migration that can exacerbate IBD. Ultimately, more data is needed before determining the efficacy of pyridoxine supplementation for active IBD.

Vitamin B₁₂ and Vitamin B₉ (Folic Acid)

Pathophysiology—Vitamin B₁₂ is reabsorbed in the terminal ileum, the distal portion of the small intestine. The American Gastroenterological Association recommends that patients with a history of extensive ileal disease or prior ileal surgery, which is the case for many patients with Crohn disease, be monitored for vitamin B₁₂ deficiency.²³ Monitoring and rapid supplementation of vitamin B₁₂ can prevent pernicious anemia and irreversible neurologic damage that may result from deficiency.⁸⁴

Folic acid is primarily absorbed in the duodenum and jejunum of the small intestine. A meta-analysis performed in 2017 assessed studies observing folic acid and vitamin B₁₂ levels in 1086 patients with IBD compared with 1484 healthy controls and found an average difference in serum folate concentration of 0.46 nmol/L (P<.001).⁸⁴ Interestingly, this study did not find a significant difference in serum vitamin B₁₂ levels between patients with IBD and healthy controls, highlighting the mechanism of vitamin B₁₂ deficiency in IBD because only patients with terminal ileal involvement are at risk for malabsorption and subsequent deficiency.

Cutaneous Manifestations—Both vitamin B₁₂ and folic acid deficiency can manifest as cheilitis, glossitis, and/or generalized hyperpigmentation that is accentuated in the flexural areas, palms, soles, and oral cavity.^85,86 Systemic symptoms of patients with vitamin B₁₂ and folic acid deficiency include megaloblastic anemia, pallor, and fatigue. A potential mechanism for the hyperpigmentation observed from vitamin B₁₂ deficiency came from an electron microscope study that showed an increased concentration of melanosomes in a patient with deficiency.⁸⁷

Diagnosis and Monitoring—In patients with suspected vitamin B₁₂ and/or folic acid deficiency, initial evaluation should include a CBC with peripheral smear and serum vitamin B₁₂ and folate levels. In cases for which the diagnosis still is unclear after initial testing, methylmalonic acid and homocysteine levels can help differentiate between the 2 deficiencies. Methylmalonic acid classically is elevated (>260 nmol/L) in vitamin B₁₂ deficiency but not in folate deficiency.⁸⁸ Cut-off values for vitamin B₁₂ deficiency are less than 200 to 250 pg/mL forserum vitamin B₁₂ and/or an elevated level of methylmalonic acid (>0.271 µmol/L).⁸⁹ A serum folic acid value greater than 3 ng/mL and/or erythrocyte folate concentrations greater than 140 ng/mL are considered adequate, whereas an indicator of folic acid deficiency is a homocysteine level less than 10 µmol/L.⁹⁰ A CBC can screen for macrocytic megaloblastic anemias (mean corpuscular volume >100 fl), which are classic diagnostic signs of an underlying vitamin B₁₂ or folate deficiency.

Treatment—According to the Centers for Disease Control and Prevention, supplementation of vitamin B₁₂ can be done orally with 1000 µg daily in patients with deficiency. In patients with active IBD, oral reabsorption of vitamin B₁₂ can be less effective, making subcutaneous or intramuscular administration (1000 µg/wk for 8 weeks, then monthly for life) better options.⁸⁹

Patients with IBD managed with methotrexate should be screened carefully for folate deficiency. Methotrexate is a folate analog that sometimes is used for the treatment of IBD. Reversible competitive inhibition of dihydrofolate reductase can precipitate a systemic folic acid decrease.⁹¹ Typically, oral folic acid (1 to 5 mg/d) is sufficient to treat folate deficiency, with the ESPEN recommending 5 mg once weekly 24 to 72 hours after methotrexate treatment or 1 mg daily for 5 days per week in patients with IBD.¹ Alternative formulations—IV, subcutaneous, or intramuscular—are available for patients who cannot tolerate oral intake.⁹²

Final Thoughts

Dermatologists can be the first to observe the cutaneous manifestations of micronutrient deficiencies. Although the symptoms of each micronutrient deficiency discussed may overlap, attention to small clinical clues in patients with IBD can improve patient outcomes and quality of life. For example, koilonychia with glossitis and xerosis likely is due to iron deficiency, while zinc deficiency should be suspected in patients with scaly eczematous plaques in skin folds. A high level of suspicion for micronutrient deficiencies in patients with IBD should be followed by a complete patient history, review of systems, and thorough clinical examination. A thorough laboratory evaluation can pinpoint nutritional deficiencies in patients with IBD, keeping in mind that specific biomarkers such as ferritin and serum zinc also act as acute phase reactants and should be interpreted in this context. Co-management with gastroenterologists should be a priority in patients with IBD, as gaining control of inflammatory disease is crucial for the prevention of recurrent vitamin and micronutrient deficiencies in addition to long-term health in this population.

In 2023, ESPEN (the European Society for Clinical Nutrition and Metabolism) published consensus recommendations highlighting the importance of regular monitoring and treatment of nutrient deficiencies in patients with inflammatory bowel disease (IBD) for improved prognosis, mortality, and quality of life.¹ Suboptimal nutrition in patients with IBD predominantly results from inflammation of the gastrointestinal (GI) tract leading to malabsorption; however, medications commonly used to manage IBD also can contribute to malnutrition.^2,3 Additionally, patients may develop nausea and food avoidance due to medication or the disease itself, leading to nutritional withdrawal and eventual deficiency.⁴ Even with the development of diets focused on balancing nutritional needs and decreasing inflammation,⁵ offsetting this aversion to food can be difficult to overcome.²

Cutaneous manifestations of IBD are multifaceted and can be secondary to the disease, reactive to or associated with IBD, or effects from nutritional deficiencies. The most common vitamin and nutrient deficiencies in patients with IBD include iron; zinc; calcium; vitamin D; and vitamins B₆ (pyridoxine), B₉ (folic acid), and B₁₂.⁶ Malnutrition may manifest with cutaneous disease, and dermatologists can be the first to identify and assess for nutritional deficiencies. In this article, we review the mechanisms of these micronutrient depletions in the context of IBD, their subsequent dermatologic manifestations (Table), and treatment and monitoring guidelines for each deficiency.

Iron

A systematic review conducted from 2007 to 2012 in European patients with IBD (N=2192) found the overall prevalence of anemia in this population to be 24% (95% CI, 18%-31%), with 57% of patients with anemia experiencing iron deficiency.⁷ Anemia is observed more commonly in patients hospitalized with IBD and is common in patients with both Crohn disease and ulcerative colitis.⁸

Pathophysiology—Iron is critically important in oxygen transportation throughout the body as a major component of hemoglobin. Physiologically, the low pH of the duodenum and proximal jejunum allows divalent metal transporter 1 to transfer dietary Fe³⁺ into enterocytes, where it is reduced to the transportable Fe²⁺.^9,10 Distribution of Fe²⁺ ions from enterocytes relies on ferroportin, an iron-transporting protein, which is heavily regulated by the protein hepcidin.¹¹ Hepcidin, a known acute phase reactant, will increase in the setting of active IBD, causing a depletion of ferroportin and an inability of the body to utilize the stored iron in enterocytes.¹² This poor utilization of iron stores combined with blood loss caused by inflammation in the GI tract is the proposed primary mechanism of iron-deficiency anemia observed in patients with IBD.¹³

Cutaneous Manifestations—From a dermatologic perspective, iron-deficiency anemia can manifest with a wide range of symptoms including glossitis, koilonychia, xerosis and/or pruritus, and brittle hair or hair loss.^14,15 Although the underlying pathophysiology of these cutaneous manifestations is not fully understood, there are several theories assessing the mechanisms behind the skin findings of iron deficiency.

Atrophic glossitis has been observed in many patients with iron deficiency and is thought to manifest due to low iron concentrations in the blood, thereby decreasing oxygen delivery to the papillae of the dorsal tongue with resultant atrophy.^16,17 Similarly, decreased oxygen delivery to the nail bed capillaries may cause deformities in the nail called koilonychia (or “spoon nails”).¹⁸ Iron is a key co-factor in collagen lysyl hydroxylase that promotes collagen binding; iron deficiency may lead to disruptions in the epidermal barrier that can cause pruritus and xerosis.¹⁹ An observational study of 200 healthy patients with a primary concern of pruritus found a correlation between low serum ferritin and a higher degree of pruritus (r=−0.768; P<.00001).²⁰

Evidence for iron’s role in hair growth comes from a mouse model study with a mutation in the serine protease TMPRSS6—a protein that regulates hepcidin and iron absorption—which caused an increase in hepcidin production and subsequent systemic iron deficiency. Mice at 4 weeks of age were devoid of all body hair but had substantial regrowth after initiation of a 2-week iron-rich diet, which suggests a connection between iron repletion and hair growth in mice with iron deficiency.²¹ Additionally, a meta-analysis analyzing the comorbidities of patients with alopecia areata found them to have higher odds (odds ratio [OR]=2.78; 95% CI, 1.23-6.29) of iron-deficiency anemia but no association with IBD (OR=1.48; 95% CI, 0.32-6.82).²²

Diagnosis and Monitoring—The American Gastroenterological Association recommends a complete blood cell count (CBC), serum ferritin, transferrin saturation (TfS), and C-reactive protein (CRP) as standard evaluations for iron deficiency in patients with IBD. Patients with active IBD should be screened every 3 months,and patients with inactive disease should be screened every 6 to 12 months.²³

Although ferritin and TfS often are used as markers for iron status in healthy individuals, they are positive and negative acute phase reactants, respectively. Using them to assess iron status in patients with IBD may inaccurately represent iron status in the setting of inflammation from the disease.²⁴ The European Crohn’s and Colitis Organisation (ECCO) produced guidelines to define iron deficiency as a TfS less than 20% or a ferritin level less than 30 µg/L in patients without evidence of active IBD and a ferritin level less than 100 µg/L for patients with active inflammation.²⁵

A 2020 multicenter observational study of 202 patients with diagnosed IBD found that the ECCO guideline of ferritin less than 30 µg/L had an area under the receiver operating characteristic (AUROC) curve of 0.69, a sensitivity of 0.43, and a specificity of 0.95 in their population.²⁶ In a sensitivity analysis stratifying patients by CRP level (<10 or ≥10 mg/L), the authors found that for patients with ulcerative colitis and a CRP less than 10 mg/L, a cut-off value of ferritin less than 65 µg/L (AUROC=0.78) had a sensitivity of 0.78 and specificity of 0.76, and a TfS value of less than 16% (AUROC=0.88) had a sensitivity of 0.79 and a specificity of 0.9. In patients with a CRP of 10 mg/L or greater, a cut-off value of ferritin 80 µg/L (AUROC=0.76) had a sensitivity of 0.75 and a specificity of 0.82, and a TfS value of less than 11% (AUROC=0.69) had a sensitivity of 0.79 and a specificity of 0.88. There were no ferritin cut-off values associated with good diagnostic performance (defined as both sensitivity and specificity >0.70) for iron deficiency in patients with Crohn disease.²⁶

The authors recommended using an alternative iron measurement such as soluble transferrin receptor (sTfR)/log ferritin ratio (TfR-F) that is not influenced by active inflammation and has a good correlation with ferritin values (TfR-F: r=0.66; P<.001).²⁶ However, both sTfR and TfR-F have high costs and intermethod variability as well as differences in their reference ranges depending on which laboratory performs the analysis, limiting the accessibility and practicality of easily obtaining these tests.²⁷ Although there may be inaccuracies for standard ferritin or TfS under ECCO guidelines, proposed alternatives have their own limitations, which may make ferritin and TfS the most reasonable evaluations of iron status as long as disease activity status at the time of testing is taken into consideration.

Treatment—Treatment of underlying iron deficiency in patients with IBD requires reversing the cause of the deficiency and supplementing iron. In patients with IBD, the options to supplement iron may be limited by active disease, making oral intake less effective. Oral iron supplementation also is associated with notable GI adverse effects that may be exacerbated in patients with IBD. A systematic review of 43 randomized controlled trials (RCTs) evaluating GI adverse effects (eg, nausea, abdominal pain, diarrhea, constipation, and black or tarry stools) of oral ferrous sulfate compared with placebo or intravenous (IV) iron supplementation in healthy nonanemic individuals found a significant increase in GI adverse effects with oral supplementation (placebo: OR=2.32; P<.0001; IV: OR=3.05; P<.0001).²⁸

Therefore, IV iron repletion may be necessary in patients with IBD and may require numerous infusions depending on the formulation of iron. In an RCT conducted in 2011, patients with iron-deficiency anemia with quiescent or mild to moderate IBD were treated with either IV iron sulfate or ferric carboxymaltose.²⁹ With a primary end point of hemoglobin response greater than 2 g/dL, the authors found that 150 of 240 patients responded to ferric carboxymaltose vs 118 of 235 treated with iron sulfate (P=.004). The dosing for ferric carboxymaltose was 1 to 3 infusions of 500 to 1000 mg of iron and for iron sulfate up to 11 infusions of 200 mg of iron.²⁹

Zinc

A systematic review of zinc deficiency in patients with IBD identified 7 studies including 2413 patients and revealed those with Crohn disease had a higher prevalence of zinc deficiency compared with patients with ulcerative colitis (54% vs 41%).³⁰

Pathophysiology—Zinc serves as a catalytic cofactor for enzymatic activity within proteins and immune cells.³¹ The homeostasis of zinc is tightly regulated within the brush border of the small intestine by zinc transporters ZIP4 and ZIP1 from the lumen of enterocytes into the bloodstream.³² Inflammation in the small intestine due to Crohn disease can result in zinc malabsorption.

Ranaldi et al³³ exposed intestinal cells and zinc-depleted intestinal cells to tumor necrosis factor α media to simulate an inflammatory environment. They measured transepithelial electrical resistance as a surrogate for transmembrane permeability and found that zinc-depleted cells had a statistically significantly higher transepithelial electrical resistance percentage (60% reduction after 4 hours; P<1.10^–6) when exposed to tumor necrosis factor α signaling compared with normal intestinal cells. They concluded that zinc deficiency can increase intestinal permeability in the presence of inflammation, creating a cycle of further nutrient malabsorption and inflammation exacerbating IBD symptoms.³³

Cutaneous Manifestations—After absorption in the small intestine, approximately 5% of zinc resides in the skin, with the highest concentration in the stratum spinosum.³⁴ A cell study found that keratinocytes in zinc-deficient environments had higher rates of apoptosis compared with cells in normal media. The authors proposed that this higher rate of apoptosis and the resulting inflammation could be a mechanism for developing the desquamative or eczematous scaly plaques that are common cutaneous manifestations of zinc deficiency.³⁵

Other cutaneous findings may include angular cheilitis, stomatitis, glossitis, paronychia, onychodystrophy, generalized alopecia, and delayed wound healing.³⁶ The histopathology of these skin lesions is characterized by granular layer loss, epidermal pallor, confluent parakeratosis, spongiosis, dyskeratosis, and psoriasiform hyperplasia.³⁷

Diagnosis and Monitoring—Assessing serum zinc levels is challenging, as they may decrease during states of inflammation.³⁸ A mouse model study showed a 3.1-fold increase (P<.001) in ZIP14 expression in wild-type mice compared with an IL-6 -/- knock-down model after IL-6 exposure. The authors concluded that the upregulation of ZIP14 in the liver due to inflammatory cytokine upregulation decreases zinc availability in serum.³⁹ Additionally, serum zinc can overestimate the level of deficiency in IBD because approximately 75% of serum zinc is bound to albumin, which decreases in the setting of inflammation.^40-42

Alternatively, alkaline phosphatase (AP), a zinc-dependent metalloenzyme, may be a better evaluator of zinc status during periods of inflammation. A study in rats evaluated zinc through serum zinc levels and AP levels after a period of induced stress to mimic a short-term inflammatory state.⁴³ The researchers found that total body stores of zinc were unaffected throughout the experiment; only serum zinc declined throughout the experiment duration while AP did not. Because approximately 75% of serum zinc is bound to serum albumin,⁴² the researchers concluded the induced inflammatory state depleted serum albumin and redistributed zinc to the liver, causing the observed serum zinc changes, while total body zinc levels and AP were largely unaffected in comparison.⁴³ Comorbid conditions such as liver or bone disease can increase AP levels, which limits the utility of AP as a surrogate for zinc in patients with comorbidities.⁴⁴ However, even in the context of active IBD, serum zinc still is currently considered the best biomarker to evaluate zinc status.⁴⁵

Treatment—The recommended dose for zinc supplementation is 20 to 40 mg daily with higher doses (>50 mg/d) for patients with malabsorptive syndromes such as IBD.⁴⁶ It can be administered orally or parenterally. Although rare, zinc replacement therapy may be associated with diarrhea, nausea, vomiting, mild headaches, and fatigue.⁴⁶ Additional considerations should be taken when repleting other micronutrients with zinc, as calcium and folate can inhibit zinc reabsorption, while zinc itself can inhibit iron and copper reabsorption.⁴⁷

Vitamin D and Calcium

Low vitamin D levels (<50 nmol/L) and hypocalcemia (<8.8 mg/dL) are common in patients with IBD.^48,49

Pathophysiology—Vitamin D levels are maintained via 2 mechanisms. The first mechanism is through the skin, as keratinocytes produce 7-dehydrocholesterol after exposure to UV light, which is converted into previtamin D₃ and then thermally isomerizes into vitamin D₃. This vitamin D₃ is then transported to the liver on vitamin D–binding protein.⁵⁰ The second mechanism is through oral vitamin D₃ that is absorbed through vitamin D receptors in intestinal epithelium and transported to the liver, where it is hydroxylated into 25-hydroxyvitamin D (25[OH]D), then to the kidneys for hydroxylation to 1,25(OH)₂D for redistribution throughout the body.⁵⁰ This activated form of vitamin D regulates calcium absorption in the intestine, and optimal vitamin D levels are necessary to absorb calcium efficiently.⁵¹ Inflammation from IBD within the small intestine can downregulate vitamin D receptors, causing malabsorption and decreased serum vitamin D.⁵²

Vitamin D signaling also is vital to maintaining the tight junctions and adherens junctions of the intestinal epithelium. Weakening the permeability of the epithelium further exacerbates malabsorption and subsequent vitamin D deficiency.⁵² A meta-analysis of 27 studies including 8316 patients with IBD showed low vitamin D levels were associated with increased odds of disease activity (OR=1.53; 95% CI, 1.32-1.77), mucosal inflammation (OR=1.25; 95% CI, 1.06-1.47), and future clinical relapse (OR=1.23; 95% CI, 1.03-1.47) in patients with Crohn disease. The authors concluded that low levels of vitamin D could be used as a potential biomarker of inflammatory status in Crohn disease.⁵³

Vitamin D and calcium are further implicated in maintaining skeletal health,⁴⁷ while vitamin D specifically helps maintain intestinal homeostasis⁵⁴ and immune system modulation in the skin.⁵⁵

Cutaneous Manifestations—Vitamin D is thought to play crucial roles in skin differentiation and proliferation, cutaneous innate immunity, hair follicle cycling, photoprotection, and wound healing.⁵⁶ Vitamin D deficiency has been observed in a large range of cutaneous diseases including skin cancer, psoriasis, vitiligo, bullous pemphigoid, atopic dermatitis, and various types of alopecia.^56-59 It is unclear whether vitamin D deficiency facilitates these disease processes or is merely the consequence of a disrupted cutaneous surface with the inability to complete the first step in vitamin D processing. A 2014 meta-analysis of 290 prospective cohort studies and 172 randomized trials concluded that 25(OH)D deficiency was associated with ill health and did not find causal evidence for any specific disease, dermatologic or otherwise.⁶⁰ Calcium deficiency may cause epidermal changes including dry skin, coarse hair, and brittle nails.⁶¹

Diagnosis and Monitoring—The ECCO guidelines recommend obtaining serum 25(OH)D levels every 3 months in patients with IBD.⁶² Levels less than 75 nmol/L are considered deficient, and a value less than 30 nmol/L increases the risk for osteomalacia and nutritional rickets, constituting severe vitamin D deficiency.^63-65

An observational study of 325 patients with IBD showed a statistically significant negative correlation between serum vitamin D and fecal calprotectin (r=−0.19; P<.001), a stool-based marker for gut inflammation, supporting vitamin D as a potential biomarker in IBD.⁶⁶

Evaluation of calcium can be done through serum levels in patients with IBD.⁶⁷ Patients with IBD are at risk for hypoalbuminemia; therefore, consideration should be taken to ensure calcium levels are corrected, as approximately 50% of calcium is bound to albumin or other ions in the body,⁶⁸ which can be done by adjusting the calcium concentration by 0.02 mmol/L for every 1 g/L of albumin above or below 40 g/L. In the most critically ill patients, a direct ionized calcium blood level should be used instead because the previously mentioned correction calculations are inaccurate when albumin is critically low.⁶⁹

Treatment—The ECCO guidelines recommend calcium and vitamin D repletion of 500 to 1000 mg and 800 to 1000 U, respectively, in patients with IBD on systemic corticosteroids to prevent the negative effects of bone loss.⁶² Calcium repletion in patients with IBD who are not on systemic steroids are the same as for the general population.⁶⁵

Vitamin D repletion also may help decrease IBD activity. In a prospective study, 10,000 IU/d of vitamin D in 10 patients with IBD—adjusted over 12 weeks to a target of 100 to 125 nmol/L of serum 25(OH)D—showed a significant reduction in clinical Crohn activity (P=.019) over the study period.⁷⁰ In contrast, 2000 IU/d for 3 months in an RCT of 27 patients with Crohn disease found significantly lower CRP (P=.019) and significantly higher self-reported quality of life (P=.037) but nonsignificant decreases in Crohn activity (P=.082) in patients with 25(OH)D levels of 75 nmol/L or higher compared with those with 25(OH)D levels less than 75 nmol/L.⁷¹

These discrepancies illustrate the need for expanded clinical trials to elucidate the optimal vitamin D dosing for patients with IBD. Ultimately, assessing vitamin D and calcium status and considering repletion in patients with IBD, especially those with comorbid dermatologic diseases such as poor wound healing, psoriasis, or atopic dermatitis, is important.

Vitamin B₆ (Pyridoxine)

Pathophysiology—Pyridoxine is an important coenzyme for many functions including amino acid transamination, fatty acid metabolism, and conversion of tryptophan to niacin. It is absorbed in the jejunum and ileum and subsequently transported to the liver for rephosphorylation and release into its active form.³⁶ An observational study assessing the nutritional status of patients with IBD found that only 5.7% of 105 patients with food records had inadequate dietary intake of pyridoxine, but 29% of all patients with IBD had subnormal pyridoxine levels.⁷² Additionally, they found no significant difference in the prevalence of subnormal pyridoxine levels in patients with active IBD vs IBD in remission. The authors suggested that the subnormal pyridoxine levels in patients with IBD likely were multifactorial and resulted from malabsorption due to active disease, inflammation, and inadequate intake.⁷²

Cutaneous Manifestations—Cutaneous findings associated with pyridoxine deficiency include periorificial and perineal dermatitis,⁷³ angular stomatitis, and cheilitis with associated burning, redness, and tongue edema.³⁶ Additionally, pyridoxine is involved in the conversion of tryptophan to niacin, and its deficiency may manifest with pellagralike findings.⁷⁴

Because pyridoxine is critical to protein metabolism, its deficiency may disrupt key cellular structures that rely on protein concentrations to maintain structural integrity. One such structure in the skin that heavily relies on protein concentrations is the ground substance of the extracellular matrix—the amorphous gelatinous spaces that occupy the areas between the extracellular matrix, which consists of cross-linked glycosaminoglycans and proteins.⁷⁵ Without protein, ground substance increases in viscosity and can disrupt the epidermal barrier, leading to increased transepidermal water loss and ultimately inflammation.⁷⁶ Although this theory has yet to be validated fully, this is a potential mechanistic explanation for the inflammation in dermal papillae that leads to dermatitis observed in pyridoxine deficiency.

Diagnosis and Monitoring—Direct biomarkers of pyridoxine status are in serum, plasma, erythrocytes, and urine, with the most common measurement in plasma as pyridoxal 5′-phosphate (PLP).⁷⁷ Plasma PLP concentrations lower than 20 nmol/L are suggestive of deficiency.⁷⁸ Plasma PLP has shown inverse relationships with acute phase inflammatory markers CRP⁷⁹ and AP,⁷⁸ thereby raising concerns for its validity to assess pyridoxine status in patients with symptomatic IBD.⁸⁰

Alternative evaluations of pyridoxine include tryptophan and methionine loading tests,³⁶ which are measured via urinary excretion and require normal kidney function to be accurate. They should be considered in IBD if necessary, but routine testing, even in patients with symptomatic IBD, is not recommended in the ECCO guidelines. Additional considerations should be taken in patients with altered nutrient requirements such as those who have undergone bowel resection due to highly active disease or those who receive parenteral nutritional supplementation.⁸¹

Treatment—Recommendations for oral pyridoxine supplementation range from 25 to 600 mg daily,⁸² with symptoms typically improving on 100 mg daily.³⁶ Pyridoxine supplementation may have additional benefits for patients with IBD and potentially modulate disease severity. An IL-10 knockout mouse supplemented with pyridoxine had an approximately 60% reduction (P<.05) in inflammation compared to mice deficient in pyridoxine.⁸³ The authors suggest that PLP-dependent enzymes can inhibit further proinflammatory signaling and T-cell migration that can exacerbate IBD. Ultimately, more data is needed before determining the efficacy of pyridoxine supplementation for active IBD.

Vitamin B₁₂ and Vitamin B₉ (Folic Acid)

Pathophysiology—Vitamin B₁₂ is reabsorbed in the terminal ileum, the distal portion of the small intestine. The American Gastroenterological Association recommends that patients with a history of extensive ileal disease or prior ileal surgery, which is the case for many patients with Crohn disease, be monitored for vitamin B₁₂ deficiency.²³ Monitoring and rapid supplementation of vitamin B₁₂ can prevent pernicious anemia and irreversible neurologic damage that may result from deficiency.⁸⁴

Folic acid is primarily absorbed in the duodenum and jejunum of the small intestine. A meta-analysis performed in 2017 assessed studies observing folic acid and vitamin B₁₂ levels in 1086 patients with IBD compared with 1484 healthy controls and found an average difference in serum folate concentration of 0.46 nmol/L (P<.001).⁸⁴ Interestingly, this study did not find a significant difference in serum vitamin B₁₂ levels between patients with IBD and healthy controls, highlighting the mechanism of vitamin B₁₂ deficiency in IBD because only patients with terminal ileal involvement are at risk for malabsorption and subsequent deficiency.

Cutaneous Manifestations—Both vitamin B₁₂ and folic acid deficiency can manifest as cheilitis, glossitis, and/or generalized hyperpigmentation that is accentuated in the flexural areas, palms, soles, and oral cavity.^85,86 Systemic symptoms of patients with vitamin B₁₂ and folic acid deficiency include megaloblastic anemia, pallor, and fatigue. A potential mechanism for the hyperpigmentation observed from vitamin B₁₂ deficiency came from an electron microscope study that showed an increased concentration of melanosomes in a patient with deficiency.⁸⁷

Diagnosis and Monitoring—In patients with suspected vitamin B₁₂ and/or folic acid deficiency, initial evaluation should include a CBC with peripheral smear and serum vitamin B₁₂ and folate levels. In cases for which the diagnosis still is unclear after initial testing, methylmalonic acid and homocysteine levels can help differentiate between the 2 deficiencies. Methylmalonic acid classically is elevated (>260 nmol/L) in vitamin B₁₂ deficiency but not in folate deficiency.⁸⁸ Cut-off values for vitamin B₁₂ deficiency are less than 200 to 250 pg/mL forserum vitamin B₁₂ and/or an elevated level of methylmalonic acid (>0.271 µmol/L).⁸⁹ A serum folic acid value greater than 3 ng/mL and/or erythrocyte folate concentrations greater than 140 ng/mL are considered adequate, whereas an indicator of folic acid deficiency is a homocysteine level less than 10 µmol/L.⁹⁰ A CBC can screen for macrocytic megaloblastic anemias (mean corpuscular volume >100 fl), which are classic diagnostic signs of an underlying vitamin B₁₂ or folate deficiency.

Treatment—According to the Centers for Disease Control and Prevention, supplementation of vitamin B₁₂ can be done orally with 1000 µg daily in patients with deficiency. In patients with active IBD, oral reabsorption of vitamin B₁₂ can be less effective, making subcutaneous or intramuscular administration (1000 µg/wk for 8 weeks, then monthly for life) better options.⁸⁹

Patients with IBD managed with methotrexate should be screened carefully for folate deficiency. Methotrexate is a folate analog that sometimes is used for the treatment of IBD. Reversible competitive inhibition of dihydrofolate reductase can precipitate a systemic folic acid decrease.⁹¹ Typically, oral folic acid (1 to 5 mg/d) is sufficient to treat folate deficiency, with the ESPEN recommending 5 mg once weekly 24 to 72 hours after methotrexate treatment or 1 mg daily for 5 days per week in patients with IBD.¹ Alternative formulations—IV, subcutaneous, or intramuscular—are available for patients who cannot tolerate oral intake.⁹²

Final Thoughts

Dermatologists can be the first to observe the cutaneous manifestations of micronutrient deficiencies. Although the symptoms of each micronutrient deficiency discussed may overlap, attention to small clinical clues in patients with IBD can improve patient outcomes and quality of life. For example, koilonychia with glossitis and xerosis likely is due to iron deficiency, while zinc deficiency should be suspected in patients with scaly eczematous plaques in skin folds. A high level of suspicion for micronutrient deficiencies in patients with IBD should be followed by a complete patient history, review of systems, and thorough clinical examination. A thorough laboratory evaluation can pinpoint nutritional deficiencies in patients with IBD, keeping in mind that specific biomarkers such as ferritin and serum zinc also act as acute phase reactants and should be interpreted in this context. Co-management with gastroenterologists should be a priority in patients with IBD, as gaining control of inflammatory disease is crucial for the prevention of recurrent vitamin and micronutrient deficiencies in addition to long-term health in this population.

To the Editor:

Recurrent aphthous stomatitis (RAS) is a mucocutaneous condition characterized by single or multiple, painful,^1,2 round ulcerations of variable sizes with a tendency for recurrence, most commonly located in nonkeratinized areas of the oral mucosa. Pathergy commonly is observed.³ Although many authors consider the terms RAS andaphtha to be synonymous,^4,5 differentiating the clinical lesion (aphthous ulceration) from the disease (aphtha or RAS) can be useful, as several other diseases can at times manifest with similar ulcers (called aphthoid lesions), such as pemphigus vulgaris, mucous membrane pemphigoid, and erythema multiforme.⁶

It is estimated that approximately 20% of individuals worldwide have at least one episode of aphtha during their lifetime,⁷ and it is considered the most common disease of the oral mucosa.^8,9 However, only patients presenting with severe acute outbreaks or frequent relapses typically seek medical treatment. Clinically, aphthous ulcers are classified as aphtha minor (small number of small lesions), aphtha major (large deep lesions that also can affect the minor salivary glands with intense necrosis, difficulty in healing, and mucosal scarring), and aphtha herpetiformis (innumerous tiny lesions that reappear in recurring outbreaks).^1-3 The term complex aphthosis was introduced in 1985¹⁰ and is defined as recurrent oral and genital aphthous ulcerations or recurring multiple oral aphthous ulcers in the absence of systemic manifestations or Behçet disease^11,12; however, complex aphthosis also has been reported as frequent episodes of ulcerations that may be associated with systemic diseases including Behçet disease.^13,14

Currently, RAS is considered an immunologically mediated alteration in cutaneous mucosal reactivity with a multifactorial systemic cause. Underlying conditions such as Behçet disease, inflammatory bowel disease (IBD), iatrogenic immunosuppression (eg, following solid organ transplantation), AIDS, and cyclic neutropenia may or may not be detected.^11-13

Our retrospective study explored the systemic nature of RAS. We reviewed patient records to evaluate underlying systemic conditions associated with the diagnosis of RAS and the use of oral medications in managing the disease. Medical records from the Department of Dermatology of the University of São Paulo, Brazil, from 2003 to 2017 were reviewed to identify patients with a diagnosis of RAS. Clinical classification of RAS—minor, major, or herpetiform—as well as the presence of aphthous lesions in other locations and the presence of other associated inflammatory cutaneous manifestations also were noted. Associated systemic diseases and treatments for RAS were recorded. Patients for whom the diagnosis of RAS was changed during follow-up were excluded. Because this was a retrospective analysis of medical records and without any patient risk, informed consent was not needed.

Medical records for 125 patients were reviewed; 63 were male (50.4%), and 62 were female (49.6%). The age at onset of symptoms, which ranged from a few months after birth to 74 years, was reported in only 92 (73.6%) patient medical records. Of these, 30 (32.6%) reported onset before 20 years of age, 39 (42.4%) between 20 and 39 years, 17 (18.5%) between 40 and 59 years, and 6 (6.5%) at 60 years or older. Morphologically, 72 (57.6%) had minor, 42 (33.6%) had major, and 11 (8.8%) had herpetiform aphthous ulcers. None of the patients presented with sporadic lesions; the disease was long-standing and persistent in all cases (complex aphthosis).

Regarding the location of the ulcers, 92 (73.6%) patients had lesions on the oral mucosa only. Some patients had lesions in more than one site in addition to the oral mucosa: 32 (25.6%) had aphthae in the genital/groin region and 4 (3.2%) presented with perianal/anal aphthae. Nineteen patients (19.2%) presented other cutaneous manifestations in addition to aphthae: 11 (45.8%) had folliculitis/pseudofolliculitis, and 8 (33.3%) had erythema nodosum (EN). Eight patients (33.3%) presented with uveitis, and 6 (25%) presented with concomitant arthralgia/arthritis. Fifty-four patients (43.2%) had confirmed or suspected associated disease: Behçet disease (21 [38.9%]), IBD (10 [18.5%]), solid organ transplantation (7 [13.0%])(kidney, 4 [57.1%]; heart, 2 [28.6%]; liver, 1 [14.3%]), HIV infection (6 [11.1%]), lymphoma (1 [1.9%]), aplastic anemia (1 [1.9%]), or myelodysplastic syndrome (1 [1.9%]). Ten patients (18.5%) presented with other diseases under investigation (eg, unidentified rheumatologic disease, unexplained neutropenia, undiagnosed immunodeficiencies, autoinflammatory syndromes, possible cyclic neutropenia).

Biopsies of the oral mucosa were performed in 31 patients. Histopathologic findings will be discussed in a future publication (unpublished data).

Five patients (4.0%) were lost to follow-up and did not receive treatment; 10 (8.0%) received only topical treatment (analgesics and/or corticosteroids). All 9 (7.2%) patients undergoing intralesional corticosteroid injections also were on a systemic treatment. One hundred ten (88.0%) patients were treated systemically—with colchicine (84/110 [76.4%]), thalidomide (43/110 [39.1%]), small pulses of oral corticosteroids (26 [23.6%]), dapsone (12/110 [10.9%]), or pentoxifylline (3 [2.7%]). Furthermore, in patients with associated diseases, treatment of the underlying condition was conducted when available, and follow-up was carried out in conjunction with the appropriate specialists. For treatment of the associated disease, patients received other medications such as methotrexate, azathioprine, cyclophosphamide, intravenous corticosteroid pulse, and immunobiologics.

The prevalence of RAS between sexes in our study population was similar (50.4% male; 49.6% female). Results from prior studies have been mixed; some reported a higher prevalence in females,^15-18 while others found no predilection for sex among patients diagnosed with RAS.^19,20 In our analysis, 75% of patients experienced symptoms of RAS before 40 years of age; in prior studies, up to 56% of patients experienced symptoms between the ages of 20 and 40 years.^21,22

In our study, 26.4% of patients had extraoral aphthae. Genital lesions have been described as infrequent,²³ and lesions manifesting in other mucous membranes or on the skin are rare.²⁴ A study reported genital involvement in 8% to 13% of patients with oral aphtha.²⁵ We observed genital involvement in 25.6% of patients. Likewise, this higher value may be due to our study population of patients referred to our university hospital. In our study, 19.2% of patients presented with other inflammatory manifestations in addition to aphthous ulcerations (eg, folliculitis, EN, uveitis, arthritis). As dermatologists in a tertiary reference hospital, we actively look for such associations in every aphtha patient, which may not be the case in many nondermatologic oral care services.

In our study population, 43.2% of patients were diagnosed with or were under investigation for systemic diseases known to be associated with RAS. We found associations with Behçet disease most frequently, followed by IBD,²⁶ solid organ transplantation, and HIV. In this group of patients, the respective systemic disease was active or poorly controlled. In transplant recipients, aphtha major was the most common type, similar to other studies.²⁷ We observed no notable difference in the clinical picture of the oral ulcers in patients with a well-established systemic disease vs those without.

Most of our cases did not present findings other than aphtha, indicating that the intrinsic defect that predisposes to RAS is always systemic. Even mild and sporadic cases may be attributable to a systemic disorder of cutaneous-mucosal reactivity. The predisposition to RAS never originates in the oral cavity, hence the confusion caused and the uselessness of studies that relate aphthae to factors such as local food allergies, pH changes, or local infection with microorganisms.^5,28 The disease course (reducing the frequency of lesion appearance and accelerating the healing of extensive lesions) is only modified with systemic treatment, with local measures proving to be only moderately useful to relieve pain. We believe that RAS can in many ways be compared to EN and pyoderma gangrenosum (PG): some systemic conditions that predispose patients to EN and PG also may predispose them to RAS (eg, IBD, hematologic disorders). Similar to RAS, many cases of EN and PG are idiopathic. In addition, pathergy also occurs in PG.^11,13

We were unable to observe or establish any predictive clinical element that could indicate a better or worse response to the prescribed treatments, which also has been noted by other authors.^3,4 Treatment of RAS is empiric, generally starting with drugs that are easier to prescribe and with fewer adverse effects, then progressing to more complex drugs when a good response is not obtained. Colchicine was the most commonly prescribed medication (76.4% [84/110]). It has been proposed by several authors^3,4 as a first-line systemic medication for the treatment of recurrent aphthae, as it has been shown to be effective and safe. The dosage ranged from 0.5 mg twice daily to 0.5 mg 4 times daily. Dapsone is an established drug for aphtha^29,30 and was used in 12 of our patients. The dosage used in our patients ranged from 50 to 100 mg/d. Adverse effects such as hemolytic anemia frequently are seen, and one of the patients in our study developed DRESS (drug reaction with eosinophilia and systemic symptoms) syndrome in response to dapsone. In 7 cases, colchicine and dapsone were used together, which is believed to potentiate the therapeutic effects. This combination may be useful in patients for whom thalidomide cannot be used or those who have not improved with monotherapy.²⁹ Thalidomide is considered one of the most effective drugs for RAS.^30,31 Forty-three patients in our analysis were treated with thalidomide,usually as a first choice. The dosage ranged from 100 to 200 mg/d. It was mainly chosen in disabling pediatric cases, adult men with aphthous major, and women with no risk for pregnancy. Due to its potential adverse effects, thalidomide has been recommended when there is no response with other medications that are dose dependent; severe adverse effects such as thromboembolism and peripheral neuropathy are rare.³¹ Oral corticosteroids were used in 26 patients, aiming at rapid improvement in very symptomatic cases; however, due to the potential for long-term adverse effects, in all cases they were prescribed in combination with another medication that was maintained after the corticosteroid was discontinued.

We highlight the systemic nature of RAS as well as its frequent association with systemic diseases and other correlated manifestations (pustules, EN, arthralgia). We also emphasize the importance of using oral medications to adequately control the disease and do not recommend topical medications aimed at treating local causes. Dermatologists should be consulted in managing severe cases of RAS.

To the Editor:

Recurrent aphthous stomatitis (RAS) is a mucocutaneous condition characterized by single or multiple, painful,^1,2 round ulcerations of variable sizes with a tendency for recurrence, most commonly located in nonkeratinized areas of the oral mucosa. Pathergy commonly is observed.³ Although many authors consider the terms RAS andaphtha to be synonymous,^4,5 differentiating the clinical lesion (aphthous ulceration) from the disease (aphtha or RAS) can be useful, as several other diseases can at times manifest with similar ulcers (called aphthoid lesions), such as pemphigus vulgaris, mucous membrane pemphigoid, and erythema multiforme.⁶

It is estimated that approximately 20% of individuals worldwide have at least one episode of aphtha during their lifetime,⁷ and it is considered the most common disease of the oral mucosa.^8,9 However, only patients presenting with severe acute outbreaks or frequent relapses typically seek medical treatment. Clinically, aphthous ulcers are classified as aphtha minor (small number of small lesions), aphtha major (large deep lesions that also can affect the minor salivary glands with intense necrosis, difficulty in healing, and mucosal scarring), and aphtha herpetiformis (innumerous tiny lesions that reappear in recurring outbreaks).^1-3 The term complex aphthosis was introduced in 1985¹⁰ and is defined as recurrent oral and genital aphthous ulcerations or recurring multiple oral aphthous ulcers in the absence of systemic manifestations or Behçet disease^11,12; however, complex aphthosis also has been reported as frequent episodes of ulcerations that may be associated with systemic diseases including Behçet disease.^13,14

Currently, RAS is considered an immunologically mediated alteration in cutaneous mucosal reactivity with a multifactorial systemic cause. Underlying conditions such as Behçet disease, inflammatory bowel disease (IBD), iatrogenic immunosuppression (eg, following solid organ transplantation), AIDS, and cyclic neutropenia may or may not be detected.^11-13

Our retrospective study explored the systemic nature of RAS. We reviewed patient records to evaluate underlying systemic conditions associated with the diagnosis of RAS and the use of oral medications in managing the disease. Medical records from the Department of Dermatology of the University of São Paulo, Brazil, from 2003 to 2017 were reviewed to identify patients with a diagnosis of RAS. Clinical classification of RAS—minor, major, or herpetiform—as well as the presence of aphthous lesions in other locations and the presence of other associated inflammatory cutaneous manifestations also were noted. Associated systemic diseases and treatments for RAS were recorded. Patients for whom the diagnosis of RAS was changed during follow-up were excluded. Because this was a retrospective analysis of medical records and without any patient risk, informed consent was not needed.

Medical records for 125 patients were reviewed; 63 were male (50.4%), and 62 were female (49.6%). The age at onset of symptoms, which ranged from a few months after birth to 74 years, was reported in only 92 (73.6%) patient medical records. Of these, 30 (32.6%) reported onset before 20 years of age, 39 (42.4%) between 20 and 39 years, 17 (18.5%) between 40 and 59 years, and 6 (6.5%) at 60 years or older. Morphologically, 72 (57.6%) had minor, 42 (33.6%) had major, and 11 (8.8%) had herpetiform aphthous ulcers. None of the patients presented with sporadic lesions; the disease was long-standing and persistent in all cases (complex aphthosis).

Regarding the location of the ulcers, 92 (73.6%) patients had lesions on the oral mucosa only. Some patients had lesions in more than one site in addition to the oral mucosa: 32 (25.6%) had aphthae in the genital/groin region and 4 (3.2%) presented with perianal/anal aphthae. Nineteen patients (19.2%) presented other cutaneous manifestations in addition to aphthae: 11 (45.8%) had folliculitis/pseudofolliculitis, and 8 (33.3%) had erythema nodosum (EN). Eight patients (33.3%) presented with uveitis, and 6 (25%) presented with concomitant arthralgia/arthritis. Fifty-four patients (43.2%) had confirmed or suspected associated disease: Behçet disease (21 [38.9%]), IBD (10 [18.5%]), solid organ transplantation (7 [13.0%])(kidney, 4 [57.1%]; heart, 2 [28.6%]; liver, 1 [14.3%]), HIV infection (6 [11.1%]), lymphoma (1 [1.9%]), aplastic anemia (1 [1.9%]), or myelodysplastic syndrome (1 [1.9%]). Ten patients (18.5%) presented with other diseases under investigation (eg, unidentified rheumatologic disease, unexplained neutropenia, undiagnosed immunodeficiencies, autoinflammatory syndromes, possible cyclic neutropenia).

Biopsies of the oral mucosa were performed in 31 patients. Histopathologic findings will be discussed in a future publication (unpublished data).

Five patients (4.0%) were lost to follow-up and did not receive treatment; 10 (8.0%) received only topical treatment (analgesics and/or corticosteroids). All 9 (7.2%) patients undergoing intralesional corticosteroid injections also were on a systemic treatment. One hundred ten (88.0%) patients were treated systemically—with colchicine (84/110 [76.4%]), thalidomide (43/110 [39.1%]), small pulses of oral corticosteroids (26 [23.6%]), dapsone (12/110 [10.9%]), or pentoxifylline (3 [2.7%]). Furthermore, in patients with associated diseases, treatment of the underlying condition was conducted when available, and follow-up was carried out in conjunction with the appropriate specialists. For treatment of the associated disease, patients received other medications such as methotrexate, azathioprine, cyclophosphamide, intravenous corticosteroid pulse, and immunobiologics.

The prevalence of RAS between sexes in our study population was similar (50.4% male; 49.6% female). Results from prior studies have been mixed; some reported a higher prevalence in females,^15-18 while others found no predilection for sex among patients diagnosed with RAS.^19,20 In our analysis, 75% of patients experienced symptoms of RAS before 40 years of age; in prior studies, up to 56% of patients experienced symptoms between the ages of 20 and 40 years.^21,22

In our study, 26.4% of patients had extraoral aphthae. Genital lesions have been described as infrequent,²³ and lesions manifesting in other mucous membranes or on the skin are rare.²⁴ A study reported genital involvement in 8% to 13% of patients with oral aphtha.²⁵ We observed genital involvement in 25.6% of patients. Likewise, this higher value may be due to our study population of patients referred to our university hospital. In our study, 19.2% of patients presented with other inflammatory manifestations in addition to aphthous ulcerations (eg, folliculitis, EN, uveitis, arthritis). As dermatologists in a tertiary reference hospital, we actively look for such associations in every aphtha patient, which may not be the case in many nondermatologic oral care services.

In our study population, 43.2% of patients were diagnosed with or were under investigation for systemic diseases known to be associated with RAS. We found associations with Behçet disease most frequently, followed by IBD,²⁶ solid organ transplantation, and HIV. In this group of patients, the respective systemic disease was active or poorly controlled. In transplant recipients, aphtha major was the most common type, similar to other studies.²⁷ We observed no notable difference in the clinical picture of the oral ulcers in patients with a well-established systemic disease vs those without.

Most of our cases did not present findings other than aphtha, indicating that the intrinsic defect that predisposes to RAS is always systemic. Even mild and sporadic cases may be attributable to a systemic disorder of cutaneous-mucosal reactivity. The predisposition to RAS never originates in the oral cavity, hence the confusion caused and the uselessness of studies that relate aphthae to factors such as local food allergies, pH changes, or local infection with microorganisms.^5,28 The disease course (reducing the frequency of lesion appearance and accelerating the healing of extensive lesions) is only modified with systemic treatment, with local measures proving to be only moderately useful to relieve pain. We believe that RAS can in many ways be compared to EN and pyoderma gangrenosum (PG): some systemic conditions that predispose patients to EN and PG also may predispose them to RAS (eg, IBD, hematologic disorders). Similar to RAS, many cases of EN and PG are idiopathic. In addition, pathergy also occurs in PG.^11,13

We were unable to observe or establish any predictive clinical element that could indicate a better or worse response to the prescribed treatments, which also has been noted by other authors.^3,4 Treatment of RAS is empiric, generally starting with drugs that are easier to prescribe and with fewer adverse effects, then progressing to more complex drugs when a good response is not obtained. Colchicine was the most commonly prescribed medication (76.4% [84/110]). It has been proposed by several authors^3,4 as a first-line systemic medication for the treatment of recurrent aphthae, as it has been shown to be effective and safe. The dosage ranged from 0.5 mg twice daily to 0.5 mg 4 times daily. Dapsone is an established drug for aphtha^29,30 and was used in 12 of our patients. The dosage used in our patients ranged from 50 to 100 mg/d. Adverse effects such as hemolytic anemia frequently are seen, and one of the patients in our study developed DRESS (drug reaction with eosinophilia and systemic symptoms) syndrome in response to dapsone. In 7 cases, colchicine and dapsone were used together, which is believed to potentiate the therapeutic effects. This combination may be useful in patients for whom thalidomide cannot be used or those who have not improved with monotherapy.²⁹ Thalidomide is considered one of the most effective drugs for RAS.^30,31 Forty-three patients in our analysis were treated with thalidomide,usually as a first choice. The dosage ranged from 100 to 200 mg/d. It was mainly chosen in disabling pediatric cases, adult men with aphthous major, and women with no risk for pregnancy. Due to its potential adverse effects, thalidomide has been recommended when there is no response with other medications that are dose dependent; severe adverse effects such as thromboembolism and peripheral neuropathy are rare.³¹ Oral corticosteroids were used in 26 patients, aiming at rapid improvement in very symptomatic cases; however, due to the potential for long-term adverse effects, in all cases they were prescribed in combination with another medication that was maintained after the corticosteroid was discontinued.

We highlight the systemic nature of RAS as well as its frequent association with systemic diseases and other correlated manifestations (pustules, EN, arthralgia). We also emphasize the importance of using oral medications to adequately control the disease and do not recommend topical medications aimed at treating local causes. Dermatologists should be consulted in managing severe cases of RAS.

To the Editor:

Recurrent aphthous stomatitis (RAS) is a mucocutaneous condition characterized by single or multiple, painful,^1,2 round ulcerations of variable sizes with a tendency for recurrence, most commonly located in nonkeratinized areas of the oral mucosa. Pathergy commonly is observed.³ Although many authors consider the terms RAS andaphtha to be synonymous,^4,5 differentiating the clinical lesion (aphthous ulceration) from the disease (aphtha or RAS) can be useful, as several other diseases can at times manifest with similar ulcers (called aphthoid lesions), such as pemphigus vulgaris, mucous membrane pemphigoid, and erythema multiforme.⁶

It is estimated that approximately 20% of individuals worldwide have at least one episode of aphtha during their lifetime,⁷ and it is considered the most common disease of the oral mucosa.^8,9 However, only patients presenting with severe acute outbreaks or frequent relapses typically seek medical treatment. Clinically, aphthous ulcers are classified as aphtha minor (small number of small lesions), aphtha major (large deep lesions that also can affect the minor salivary glands with intense necrosis, difficulty in healing, and mucosal scarring), and aphtha herpetiformis (innumerous tiny lesions that reappear in recurring outbreaks).^1-3 The term complex aphthosis was introduced in 1985¹⁰ and is defined as recurrent oral and genital aphthous ulcerations or recurring multiple oral aphthous ulcers in the absence of systemic manifestations or Behçet disease^11,12; however, complex aphthosis also has been reported as frequent episodes of ulcerations that may be associated with systemic diseases including Behçet disease.^13,14

Currently, RAS is considered an immunologically mediated alteration in cutaneous mucosal reactivity with a multifactorial systemic cause. Underlying conditions such as Behçet disease, inflammatory bowel disease (IBD), iatrogenic immunosuppression (eg, following solid organ transplantation), AIDS, and cyclic neutropenia may or may not be detected.^11-13

Our retrospective study explored the systemic nature of RAS. We reviewed patient records to evaluate underlying systemic conditions associated with the diagnosis of RAS and the use of oral medications in managing the disease. Medical records from the Department of Dermatology of the University of São Paulo, Brazil, from 2003 to 2017 were reviewed to identify patients with a diagnosis of RAS. Clinical classification of RAS—minor, major, or herpetiform—as well as the presence of aphthous lesions in other locations and the presence of other associated inflammatory cutaneous manifestations also were noted. Associated systemic diseases and treatments for RAS were recorded. Patients for whom the diagnosis of RAS was changed during follow-up were excluded. Because this was a retrospective analysis of medical records and without any patient risk, informed consent was not needed.

Medical records for 125 patients were reviewed; 63 were male (50.4%), and 62 were female (49.6%). The age at onset of symptoms, which ranged from a few months after birth to 74 years, was reported in only 92 (73.6%) patient medical records. Of these, 30 (32.6%) reported onset before 20 years of age, 39 (42.4%) between 20 and 39 years, 17 (18.5%) between 40 and 59 years, and 6 (6.5%) at 60 years or older. Morphologically, 72 (57.6%) had minor, 42 (33.6%) had major, and 11 (8.8%) had herpetiform aphthous ulcers. None of the patients presented with sporadic lesions; the disease was long-standing and persistent in all cases (complex aphthosis).

Regarding the location of the ulcers, 92 (73.6%) patients had lesions on the oral mucosa only. Some patients had lesions in more than one site in addition to the oral mucosa: 32 (25.6%) had aphthae in the genital/groin region and 4 (3.2%) presented with perianal/anal aphthae. Nineteen patients (19.2%) presented other cutaneous manifestations in addition to aphthae: 11 (45.8%) had folliculitis/pseudofolliculitis, and 8 (33.3%) had erythema nodosum (EN). Eight patients (33.3%) presented with uveitis, and 6 (25%) presented with concomitant arthralgia/arthritis. Fifty-four patients (43.2%) had confirmed or suspected associated disease: Behçet disease (21 [38.9%]), IBD (10 [18.5%]), solid organ transplantation (7 [13.0%])(kidney, 4 [57.1%]; heart, 2 [28.6%]; liver, 1 [14.3%]), HIV infection (6 [11.1%]), lymphoma (1 [1.9%]), aplastic anemia (1 [1.9%]), or myelodysplastic syndrome (1 [1.9%]). Ten patients (18.5%) presented with other diseases under investigation (eg, unidentified rheumatologic disease, unexplained neutropenia, undiagnosed immunodeficiencies, autoinflammatory syndromes, possible cyclic neutropenia).

Biopsies of the oral mucosa were performed in 31 patients. Histopathologic findings will be discussed in a future publication (unpublished data).

Five patients (4.0%) were lost to follow-up and did not receive treatment; 10 (8.0%) received only topical treatment (analgesics and/or corticosteroids). All 9 (7.2%) patients undergoing intralesional corticosteroid injections also were on a systemic treatment. One hundred ten (88.0%) patients were treated systemically—with colchicine (84/110 [76.4%]), thalidomide (43/110 [39.1%]), small pulses of oral corticosteroids (26 [23.6%]), dapsone (12/110 [10.9%]), or pentoxifylline (3 [2.7%]). Furthermore, in patients with associated diseases, treatment of the underlying condition was conducted when available, and follow-up was carried out in conjunction with the appropriate specialists. For treatment of the associated disease, patients received other medications such as methotrexate, azathioprine, cyclophosphamide, intravenous corticosteroid pulse, and immunobiologics.

The prevalence of RAS between sexes in our study population was similar (50.4% male; 49.6% female). Results from prior studies have been mixed; some reported a higher prevalence in females,^15-18 while others found no predilection for sex among patients diagnosed with RAS.^19,20 In our analysis, 75% of patients experienced symptoms of RAS before 40 years of age; in prior studies, up to 56% of patients experienced symptoms between the ages of 20 and 40 years.^21,22

In our study, 26.4% of patients had extraoral aphthae. Genital lesions have been described as infrequent,²³ and lesions manifesting in other mucous membranes or on the skin are rare.²⁴ A study reported genital involvement in 8% to 13% of patients with oral aphtha.²⁵ We observed genital involvement in 25.6% of patients. Likewise, this higher value may be due to our study population of patients referred to our university hospital. In our study, 19.2% of patients presented with other inflammatory manifestations in addition to aphthous ulcerations (eg, folliculitis, EN, uveitis, arthritis). As dermatologists in a tertiary reference hospital, we actively look for such associations in every aphtha patient, which may not be the case in many nondermatologic oral care services.

In our study population, 43.2% of patients were diagnosed with or were under investigation for systemic diseases known to be associated with RAS. We found associations with Behçet disease most frequently, followed by IBD,²⁶ solid organ transplantation, and HIV. In this group of patients, the respective systemic disease was active or poorly controlled. In transplant recipients, aphtha major was the most common type, similar to other studies.²⁷ We observed no notable difference in the clinical picture of the oral ulcers in patients with a well-established systemic disease vs those without.

Most of our cases did not present findings other than aphtha, indicating that the intrinsic defect that predisposes to RAS is always systemic. Even mild and sporadic cases may be attributable to a systemic disorder of cutaneous-mucosal reactivity. The predisposition to RAS never originates in the oral cavity, hence the confusion caused and the uselessness of studies that relate aphthae to factors such as local food allergies, pH changes, or local infection with microorganisms.^5,28 The disease course (reducing the frequency of lesion appearance and accelerating the healing of extensive lesions) is only modified with systemic treatment, with local measures proving to be only moderately useful to relieve pain. We believe that RAS can in many ways be compared to EN and pyoderma gangrenosum (PG): some systemic conditions that predispose patients to EN and PG also may predispose them to RAS (eg, IBD, hematologic disorders). Similar to RAS, many cases of EN and PG are idiopathic. In addition, pathergy also occurs in PG.^11,13

We were unable to observe or establish any predictive clinical element that could indicate a better or worse response to the prescribed treatments, which also has been noted by other authors.^3,4 Treatment of RAS is empiric, generally starting with drugs that are easier to prescribe and with fewer adverse effects, then progressing to more complex drugs when a good response is not obtained. Colchicine was the most commonly prescribed medication (76.4% [84/110]). It has been proposed by several authors^3,4 as a first-line systemic medication for the treatment of recurrent aphthae, as it has been shown to be effective and safe. The dosage ranged from 0.5 mg twice daily to 0.5 mg 4 times daily. Dapsone is an established drug for aphtha^29,30 and was used in 12 of our patients. The dosage used in our patients ranged from 50 to 100 mg/d. Adverse effects such as hemolytic anemia frequently are seen, and one of the patients in our study developed DRESS (drug reaction with eosinophilia and systemic symptoms) syndrome in response to dapsone. In 7 cases, colchicine and dapsone were used together, which is believed to potentiate the therapeutic effects. This combination may be useful in patients for whom thalidomide cannot be used or those who have not improved with monotherapy.²⁹ Thalidomide is considered one of the most effective drugs for RAS.^30,31 Forty-three patients in our analysis were treated with thalidomide,usually as a first choice. The dosage ranged from 100 to 200 mg/d. It was mainly chosen in disabling pediatric cases, adult men with aphthous major, and women with no risk for pregnancy. Due to its potential adverse effects, thalidomide has been recommended when there is no response with other medications that are dose dependent; severe adverse effects such as thromboembolism and peripheral neuropathy are rare.³¹ Oral corticosteroids were used in 26 patients, aiming at rapid improvement in very symptomatic cases; however, due to the potential for long-term adverse effects, in all cases they were prescribed in combination with another medication that was maintained after the corticosteroid was discontinued.

We highlight the systemic nature of RAS as well as its frequent association with systemic diseases and other correlated manifestations (pustules, EN, arthralgia). We also emphasize the importance of using oral medications to adequately control the disease and do not recommend topical medications aimed at treating local causes. Dermatologists should be consulted in managing severe cases of RAS.

Vitiligo is a common acquired autoimmune disease that causes depigmented patches to develop throughout the skin , with descriptions dating back more than 3000 years to the earliest known Indian and Egyptian texts. Approximately 1.4% of the worldwide population has vitiligo,¹ and onset follows a bimodal age distribution with an early-onset population (mean age at onset, 10.3 years) as well as an adult-onset population (mean age at onset, 34 years).² Vitiligo manifests as well-defined, irregular, depigmented macules and patches surrounded by normal skin. The patches can vary in size from a few millimeters to several centimeters. There may be signs of inflammation, and the lesions can be itchy, but in most cases vitiligo is asymptomatic. In nonsegmental vitiligo, the depigmented patches are ymmetrical, can appear in any area of the body, and commonly progress slowly. In segmental vitiligo, the patches are unilateral, rarely cross the midline of the body, and are localized to one area. Segmental vitiligo commonly appears in childhood and progresses rapidly but stops abruptly within 6 to 12 months and remains stable, usually for life.³ Although the condition may be more apparent in patients with skin of color, vitiligo manifests at a similar rate in individuals of all races and ethnicities.⁴

Similar to most autoimmune diseases, vitiligo has a strong genetic predisposition. Although the overall prevalence of vitiligo is less than 2%, having a family history of vitiligo (ie, a first-degree relative with vitiligo) increases an individual’s risk to 6%, while concordance in identical twins is 23%.⁵ Beyond genetic predisposition, there is strong evidence that environmental exposures, such as hair dyes, contribute to risk for disease.⁶ Interestingly, vitiligo is associated with polyautoimmunity—the presence of multiple autoimmune diseases in a single patient,⁷ such as type 1 diabetes mellitus, rheumatoid arthritis, autoimmune thyroid disease, pernicious anemia, and Addison disease. Similar to vitiligo itself, polyautoimmunity likely is driven by a combination of genetic and environmental factors.⁵

We provide a brief overview of clinical trial results of Janus kinase (JAK) inhibitors for treating vitiligo and discuss the trial cohorts, with an emphasis on the impact of cohort demographic composition for individuals with skin of color. We recommend factors that investigators should consider to ensure equitable representation of individuals with skin of color in future clinical trials.

Autoimmune Pathogenesis and Treatment With JAK Inhibitors

Vitiligo is driven by autoreactive CD8⁺ T cells that target melanocytes and secrete IFN-g. Signaling of IFN-g occurs through the JAK–signal transducer and activator of transcription (JAK-STAT) pathway, leading to transcriptional changes that activate proinflammatory genes such as the chemokine CXCL10, which is required for the directed accumulation of melanocyte-specific CD8⁺ T cells at the epidermis where melanocytes reside.⁸ Once vitiligo has been initiated, the disease persists due to the presence of resident memory T cells that remain in the skin and destroy new melanocytes.^9,10

Given the central role of IFN-g signaling in the pathogenesis of vitiligo, drugs that inhibit JAK signaling are appealing to treat the disease. These JAK inhibitors bind to the kinase domain of JAK to prevent its activation, thus preventing downstream signaling events including STAT phosphorylation and its translocation to the nucleus, which ultimately stops the upregulation of inflammatory gene transcription. This process attenuates the autoimmune response in the skin and results in repigmentation of vitiligo lesions. In 2022, the US Food and Drug Administration approved the topical JAK inhibitor ruxolitinib for the treatment of vitiligo. Additional clinical trials have been initiated to test oral JAK inhibitors—ritlecitinib (ClinicalTrials.gov identifiers NCT06163326, NCT06072183, NCT05583526), povorcitinib (NCT04818346, NCT06113445, NCT06113471), and upadacitinib (NCT04927975, NCT06118411)—with strong results reported so far.¹¹

The effects of JAK inhibitors can be striking, as shown in the Figure. A patient of one of the authors (J.E.H.) used topical ruxolitinib on only the left arm for approximately 36 weeks and results were as expected—strong repigmentation of only the treated area, which is possible with JAK inhibitors. Indeed, 2 phase 3 studies—Topical Ruxolitinib Evaluation in Vitiligo (TRuE-V1 and TRuE-V2)—showed that approximately 30% of participants in TRuE-V1 (N=330) and 30.9% of participants in TRuE-V2 (N=344) achieved at least 75% improvement over baseline in the facial vitiligo area scoring index (VASI).¹² In the oral ritlecitinib phase 2b study, 12.1% of the 187 participants on the highest tested dose of ritlecitinib (loading dose of 200 mg/d for 28 days, followed by 50 mg/d maintenance dose) achieved at least 75% improvement over baseline in the VASI at 24 weeks.¹¹ Although this rate is lower than for topical ruxolitinib, this trial required all participants to have active disease (unlike the TRuE-V trials of ruxolitinib), which likely created a higher bar for repigmentation and thus resulted in fewer participants achieving the primary outcome at the early 6-month end point. Extension of treatment through 48 weeks demonstrated continued improvement over baseline without any evidence of plateau.¹¹ Although treatment with JAK inhibitors can result in dramatic repigmentation of vitiligo patches, it falls short of providing a permanent cure, as stopping treatment results in relapse (ie, the return of depigmented lesions).

Racial Disparities in Clinical Trials

Even though vitiligo affects all skin types and races/ethnicities with similar prevalence and severity, the proportion of individuals with darker skin types enrolled in these clinical trials fails to match their representation in the population as a whole. A study examining the prevalence of vitiligo in the United States reported that Black or African American individuals represented 15.8% of vitiligo diagnoses in the United States⁴ even though they are only 12.7% of the total US population. However, Black or African American individuals comprised only 5% of the combined participants in the TRuE-V clinical trials for topical ruxolitinib¹² and 2.7% of the participants in the phase 2b study of oral ritlecitinib.¹¹ This lack of appropriate representation is not unique to JAK inhibitors or other vitiligo trials. Indeed, the US Food and Drug Administration reported that Black or African American individuals comprised only 8% of participants for all clinical trials in 2020.¹³

Efficacy Metrics Beyond Repigmentation

Disparities in quality-of-life (QOL) metrics in diseases affecting individuals with skin of color also exist. In vitiligo, the contrast between affected and unaffected skin is greater in patients with skin of color, which means that for a given VASI score, the visibility of depigmentation as well as repigmentation may be variable among patients. Additionally, there is evidence that QOL concerns vary between patients with skin of color and those with lighter skin types. Ezzedine et al¹⁴ found that QOL concerns in vitiligo patients with darker skin focused more on appearance, while concerns in vitiligo patients with lighter skin focused more on skin cancer risk. In addition to QOL differences among individuals with different skin types, there also are well-documented differences in attitudes to vitiligo among certain ethnic or cultural groups.¹⁵ For example, the Rigveda (an ancient Hindu text) indicates that individuals with vitiligo and their progeny are disqualified from marriage. Although the JAK inhibitor clinical trials for vitiligo did not appear to show differences in the degree of repigmentation among different skin types or races/ethnicities, QOL measures were not collected as a secondary end point in these studies—despite the fact that at least 1 study had documented that QOL measures were not uniform across patients when stratified by age and extent of disease.^1,11,12 This same study also presented limited data suggestive of lower QOL in patients with the darkest skin phototype.¹

Considerations for Future Clinical Trials

It is logical to assume that every clinical trialist in dermatology seeks equitable representation among a diverse set of races, ethnicities, and skin types, but achieving this goal remains elusive. Two recent publications^16,17 outlined the challenges and examined solutions to address enrollment disparities, including several barriers to diversity among clinical trial participants: awareness of the clinical trials among minority populations; easy access to clinical trial sites; reluctance to participate because of prior experiences of discrimination, even if unrelated to clinical trials; and a lack of workforce diversity among the clinical trialist teams. To overcome these barriers, a multifaceted approach is needed that requires action at the level of the patient, provider, community, and institution. Once diverse representation is achieved, investigators should consider the need for QOL metrics as a secondary outcome in their trials, which will ensure that the intended clinical effect is matched by patient expectations across different races and ethnicities based on the potential differential impact that diseases such as vitiligo can have on patients with skin of color.

Vitiligo is a common acquired autoimmune disease that causes depigmented patches to develop throughout the skin , with descriptions dating back more than 3000 years to the earliest known Indian and Egyptian texts. Approximately 1.4% of the worldwide population has vitiligo,¹ and onset follows a bimodal age distribution with an early-onset population (mean age at onset, 10.3 years) as well as an adult-onset population (mean age at onset, 34 years).² Vitiligo manifests as well-defined, irregular, depigmented macules and patches surrounded by normal skin. The patches can vary in size from a few millimeters to several centimeters. There may be signs of inflammation, and the lesions can be itchy, but in most cases vitiligo is asymptomatic. In nonsegmental vitiligo, the depigmented patches are ymmetrical, can appear in any area of the body, and commonly progress slowly. In segmental vitiligo, the patches are unilateral, rarely cross the midline of the body, and are localized to one area. Segmental vitiligo commonly appears in childhood and progresses rapidly but stops abruptly within 6 to 12 months and remains stable, usually for life.³ Although the condition may be more apparent in patients with skin of color, vitiligo manifests at a similar rate in individuals of all races and ethnicities.⁴

Similar to most autoimmune diseases, vitiligo has a strong genetic predisposition. Although the overall prevalence of vitiligo is less than 2%, having a family history of vitiligo (ie, a first-degree relative with vitiligo) increases an individual’s risk to 6%, while concordance in identical twins is 23%.⁵ Beyond genetic predisposition, there is strong evidence that environmental exposures, such as hair dyes, contribute to risk for disease.⁶ Interestingly, vitiligo is associated with polyautoimmunity—the presence of multiple autoimmune diseases in a single patient,⁷ such as type 1 diabetes mellitus, rheumatoid arthritis, autoimmune thyroid disease, pernicious anemia, and Addison disease. Similar to vitiligo itself, polyautoimmunity likely is driven by a combination of genetic and environmental factors.⁵

We provide a brief overview of clinical trial results of Janus kinase (JAK) inhibitors for treating vitiligo and discuss the trial cohorts, with an emphasis on the impact of cohort demographic composition for individuals with skin of color. We recommend factors that investigators should consider to ensure equitable representation of individuals with skin of color in future clinical trials.

Autoimmune Pathogenesis and Treatment With JAK Inhibitors

Vitiligo is driven by autoreactive CD8⁺ T cells that target melanocytes and secrete IFN-g. Signaling of IFN-g occurs through the JAK–signal transducer and activator of transcription (JAK-STAT) pathway, leading to transcriptional changes that activate proinflammatory genes such as the chemokine CXCL10, which is required for the directed accumulation of melanocyte-specific CD8⁺ T cells at the epidermis where melanocytes reside.⁸ Once vitiligo has been initiated, the disease persists due to the presence of resident memory T cells that remain in the skin and destroy new melanocytes.^9,10

Given the central role of IFN-g signaling in the pathogenesis of vitiligo, drugs that inhibit JAK signaling are appealing to treat the disease. These JAK inhibitors bind to the kinase domain of JAK to prevent its activation, thus preventing downstream signaling events including STAT phosphorylation and its translocation to the nucleus, which ultimately stops the upregulation of inflammatory gene transcription. This process attenuates the autoimmune response in the skin and results in repigmentation of vitiligo lesions. In 2022, the US Food and Drug Administration approved the topical JAK inhibitor ruxolitinib for the treatment of vitiligo. Additional clinical trials have been initiated to test oral JAK inhibitors—ritlecitinib (ClinicalTrials.gov identifiers NCT06163326, NCT06072183, NCT05583526), povorcitinib (NCT04818346, NCT06113445, NCT06113471), and upadacitinib (NCT04927975, NCT06118411)—with strong results reported so far.¹¹

The effects of JAK inhibitors can be striking, as shown in the Figure. A patient of one of the authors (J.E.H.) used topical ruxolitinib on only the left arm for approximately 36 weeks and results were as expected—strong repigmentation of only the treated area, which is possible with JAK inhibitors. Indeed, 2 phase 3 studies—Topical Ruxolitinib Evaluation in Vitiligo (TRuE-V1 and TRuE-V2)—showed that approximately 30% of participants in TRuE-V1 (N=330) and 30.9% of participants in TRuE-V2 (N=344) achieved at least 75% improvement over baseline in the facial vitiligo area scoring index (VASI).¹² In the oral ritlecitinib phase 2b study, 12.1% of the 187 participants on the highest tested dose of ritlecitinib (loading dose of 200 mg/d for 28 days, followed by 50 mg/d maintenance dose) achieved at least 75% improvement over baseline in the VASI at 24 weeks.¹¹ Although this rate is lower than for topical ruxolitinib, this trial required all participants to have active disease (unlike the TRuE-V trials of ruxolitinib), which likely created a higher bar for repigmentation and thus resulted in fewer participants achieving the primary outcome at the early 6-month end point. Extension of treatment through 48 weeks demonstrated continued improvement over baseline without any evidence of plateau.¹¹ Although treatment with JAK inhibitors can result in dramatic repigmentation of vitiligo patches, it falls short of providing a permanent cure, as stopping treatment results in relapse (ie, the return of depigmented lesions).

Racial Disparities in Clinical Trials

Even though vitiligo affects all skin types and races/ethnicities with similar prevalence and severity, the proportion of individuals with darker skin types enrolled in these clinical trials fails to match their representation in the population as a whole. A study examining the prevalence of vitiligo in the United States reported that Black or African American individuals represented 15.8% of vitiligo diagnoses in the United States⁴ even though they are only 12.7% of the total US population. However, Black or African American individuals comprised only 5% of the combined participants in the TRuE-V clinical trials for topical ruxolitinib¹² and 2.7% of the participants in the phase 2b study of oral ritlecitinib.¹¹ This lack of appropriate representation is not unique to JAK inhibitors or other vitiligo trials. Indeed, the US Food and Drug Administration reported that Black or African American individuals comprised only 8% of participants for all clinical trials in 2020.¹³

Efficacy Metrics Beyond Repigmentation

Disparities in quality-of-life (QOL) metrics in diseases affecting individuals with skin of color also exist. In vitiligo, the contrast between affected and unaffected skin is greater in patients with skin of color, which means that for a given VASI score, the visibility of depigmentation as well as repigmentation may be variable among patients. Additionally, there is evidence that QOL concerns vary between patients with skin of color and those with lighter skin types. Ezzedine et al¹⁴ found that QOL concerns in vitiligo patients with darker skin focused more on appearance, while concerns in vitiligo patients with lighter skin focused more on skin cancer risk. In addition to QOL differences among individuals with different skin types, there also are well-documented differences in attitudes to vitiligo among certain ethnic or cultural groups.¹⁵ For example, the Rigveda (an ancient Hindu text) indicates that individuals with vitiligo and their progeny are disqualified from marriage. Although the JAK inhibitor clinical trials for vitiligo did not appear to show differences in the degree of repigmentation among different skin types or races/ethnicities, QOL measures were not collected as a secondary end point in these studies—despite the fact that at least 1 study had documented that QOL measures were not uniform across patients when stratified by age and extent of disease.^1,11,12 This same study also presented limited data suggestive of lower QOL in patients with the darkest skin phototype.¹

Considerations for Future Clinical Trials

It is logical to assume that every clinical trialist in dermatology seeks equitable representation among a diverse set of races, ethnicities, and skin types, but achieving this goal remains elusive. Two recent publications^16,17 outlined the challenges and examined solutions to address enrollment disparities, including several barriers to diversity among clinical trial participants: awareness of the clinical trials among minority populations; easy access to clinical trial sites; reluctance to participate because of prior experiences of discrimination, even if unrelated to clinical trials; and a lack of workforce diversity among the clinical trialist teams. To overcome these barriers, a multifaceted approach is needed that requires action at the level of the patient, provider, community, and institution. Once diverse representation is achieved, investigators should consider the need for QOL metrics as a secondary outcome in their trials, which will ensure that the intended clinical effect is matched by patient expectations across different races and ethnicities based on the potential differential impact that diseases such as vitiligo can have on patients with skin of color.

Vitiligo is a common acquired autoimmune disease that causes depigmented patches to develop throughout the skin , with descriptions dating back more than 3000 years to the earliest known Indian and Egyptian texts. Approximately 1.4% of the worldwide population has vitiligo,¹ and onset follows a bimodal age distribution with an early-onset population (mean age at onset, 10.3 years) as well as an adult-onset population (mean age at onset, 34 years).² Vitiligo manifests as well-defined, irregular, depigmented macules and patches surrounded by normal skin. The patches can vary in size from a few millimeters to several centimeters. There may be signs of inflammation, and the lesions can be itchy, but in most cases vitiligo is asymptomatic. In nonsegmental vitiligo, the depigmented patches are ymmetrical, can appear in any area of the body, and commonly progress slowly. In segmental vitiligo, the patches are unilateral, rarely cross the midline of the body, and are localized to one area. Segmental vitiligo commonly appears in childhood and progresses rapidly but stops abruptly within 6 to 12 months and remains stable, usually for life.³ Although the condition may be more apparent in patients with skin of color, vitiligo manifests at a similar rate in individuals of all races and ethnicities.⁴

Similar to most autoimmune diseases, vitiligo has a strong genetic predisposition. Although the overall prevalence of vitiligo is less than 2%, having a family history of vitiligo (ie, a first-degree relative with vitiligo) increases an individual’s risk to 6%, while concordance in identical twins is 23%.⁵ Beyond genetic predisposition, there is strong evidence that environmental exposures, such as hair dyes, contribute to risk for disease.⁶ Interestingly, vitiligo is associated with polyautoimmunity—the presence of multiple autoimmune diseases in a single patient,⁷ such as type 1 diabetes mellitus, rheumatoid arthritis, autoimmune thyroid disease, pernicious anemia, and Addison disease. Similar to vitiligo itself, polyautoimmunity likely is driven by a combination of genetic and environmental factors.⁵

We provide a brief overview of clinical trial results of Janus kinase (JAK) inhibitors for treating vitiligo and discuss the trial cohorts, with an emphasis on the impact of cohort demographic composition for individuals with skin of color. We recommend factors that investigators should consider to ensure equitable representation of individuals with skin of color in future clinical trials.

Autoimmune Pathogenesis and Treatment With JAK Inhibitors

Vitiligo is driven by autoreactive CD8⁺ T cells that target melanocytes and secrete IFN-g. Signaling of IFN-g occurs through the JAK–signal transducer and activator of transcription (JAK-STAT) pathway, leading to transcriptional changes that activate proinflammatory genes such as the chemokine CXCL10, which is required for the directed accumulation of melanocyte-specific CD8⁺ T cells at the epidermis where melanocytes reside.⁸ Once vitiligo has been initiated, the disease persists due to the presence of resident memory T cells that remain in the skin and destroy new melanocytes.^9,10

Given the central role of IFN-g signaling in the pathogenesis of vitiligo, drugs that inhibit JAK signaling are appealing to treat the disease. These JAK inhibitors bind to the kinase domain of JAK to prevent its activation, thus preventing downstream signaling events including STAT phosphorylation and its translocation to the nucleus, which ultimately stops the upregulation of inflammatory gene transcription. This process attenuates the autoimmune response in the skin and results in repigmentation of vitiligo lesions. In 2022, the US Food and Drug Administration approved the topical JAK inhibitor ruxolitinib for the treatment of vitiligo. Additional clinical trials have been initiated to test oral JAK inhibitors—ritlecitinib (ClinicalTrials.gov identifiers NCT06163326, NCT06072183, NCT05583526), povorcitinib (NCT04818346, NCT06113445, NCT06113471), and upadacitinib (NCT04927975, NCT06118411)—with strong results reported so far.¹¹

The effects of JAK inhibitors can be striking, as shown in the Figure. A patient of one of the authors (J.E.H.) used topical ruxolitinib on only the left arm for approximately 36 weeks and results were as expected—strong repigmentation of only the treated area, which is possible with JAK inhibitors. Indeed, 2 phase 3 studies—Topical Ruxolitinib Evaluation in Vitiligo (TRuE-V1 and TRuE-V2)—showed that approximately 30% of participants in TRuE-V1 (N=330) and 30.9% of participants in TRuE-V2 (N=344) achieved at least 75% improvement over baseline in the facial vitiligo area scoring index (VASI).¹² In the oral ritlecitinib phase 2b study, 12.1% of the 187 participants on the highest tested dose of ritlecitinib (loading dose of 200 mg/d for 28 days, followed by 50 mg/d maintenance dose) achieved at least 75% improvement over baseline in the VASI at 24 weeks.¹¹ Although this rate is lower than for topical ruxolitinib, this trial required all participants to have active disease (unlike the TRuE-V trials of ruxolitinib), which likely created a higher bar for repigmentation and thus resulted in fewer participants achieving the primary outcome at the early 6-month end point. Extension of treatment through 48 weeks demonstrated continued improvement over baseline without any evidence of plateau.¹¹ Although treatment with JAK inhibitors can result in dramatic repigmentation of vitiligo patches, it falls short of providing a permanent cure, as stopping treatment results in relapse (ie, the return of depigmented lesions).

Racial Disparities in Clinical Trials

Even though vitiligo affects all skin types and races/ethnicities with similar prevalence and severity, the proportion of individuals with darker skin types enrolled in these clinical trials fails to match their representation in the population as a whole. A study examining the prevalence of vitiligo in the United States reported that Black or African American individuals represented 15.8% of vitiligo diagnoses in the United States⁴ even though they are only 12.7% of the total US population. However, Black or African American individuals comprised only 5% of the combined participants in the TRuE-V clinical trials for topical ruxolitinib¹² and 2.7% of the participants in the phase 2b study of oral ritlecitinib.¹¹ This lack of appropriate representation is not unique to JAK inhibitors or other vitiligo trials. Indeed, the US Food and Drug Administration reported that Black or African American individuals comprised only 8% of participants for all clinical trials in 2020.¹³

Efficacy Metrics Beyond Repigmentation

Disparities in quality-of-life (QOL) metrics in diseases affecting individuals with skin of color also exist. In vitiligo, the contrast between affected and unaffected skin is greater in patients with skin of color, which means that for a given VASI score, the visibility of depigmentation as well as repigmentation may be variable among patients. Additionally, there is evidence that QOL concerns vary between patients with skin of color and those with lighter skin types. Ezzedine et al¹⁴ found that QOL concerns in vitiligo patients with darker skin focused more on appearance, while concerns in vitiligo patients with lighter skin focused more on skin cancer risk. In addition to QOL differences among individuals with different skin types, there also are well-documented differences in attitudes to vitiligo among certain ethnic or cultural groups.¹⁵ For example, the Rigveda (an ancient Hindu text) indicates that individuals with vitiligo and their progeny are disqualified from marriage. Although the JAK inhibitor clinical trials for vitiligo did not appear to show differences in the degree of repigmentation among different skin types or races/ethnicities, QOL measures were not collected as a secondary end point in these studies—despite the fact that at least 1 study had documented that QOL measures were not uniform across patients when stratified by age and extent of disease.^1,11,12 This same study also presented limited data suggestive of lower QOL in patients with the darkest skin phototype.¹

Considerations for Future Clinical Trials

It is logical to assume that every clinical trialist in dermatology seeks equitable representation among a diverse set of races, ethnicities, and skin types, but achieving this goal remains elusive. Two recent publications^16,17 outlined the challenges and examined solutions to address enrollment disparities, including several barriers to diversity among clinical trial participants: awareness of the clinical trials among minority populations; easy access to clinical trial sites; reluctance to participate because of prior experiences of discrimination, even if unrelated to clinical trials; and a lack of workforce diversity among the clinical trialist teams. To overcome these barriers, a multifaceted approach is needed that requires action at the level of the patient, provider, community, and institution. Once diverse representation is achieved, investigators should consider the need for QOL metrics as a secondary outcome in their trials, which will ensure that the intended clinical effect is matched by patient expectations across different races and ethnicities based on the potential differential impact that diseases such as vitiligo can have on patients with skin of color.

Clinical images are integral to dermatologic care, research, and education. Studies have highlighted the underrepresentation of images of skin of color (SOC) in educational materials,¹ clinical trials,² and research publications.³ Recognition of this disparity has ignited a call to action by dermatologists and dermatologic organizations to address the gap by improving the collection and use of SOC images.⁴ It is critical to remind dermatologists of the importance of properly obtaining informed consent and ensuring images are not used without a patient’s permission, as images in journal articles, conference presentations, and educational materials can be widely distributed and shared. Herein, we summarize current practices of clinical image storage and make general recommendations on how dermatologists can better protect patient privacy. Certain cultural and social factors in patients with SOC should be considered when obtaining informed consent and collecting images.

Clinical Image Acquisition

Consenting procedures are crucial components of proper image usage. However, current consenting practices are inconsistent across various platforms, including academic journals, websites, printed text, social media, and educational presentations.⁵

Current regulations for use of patient health information in the United States are governed by the Health Insurance Portability and Accountability Act (HIPAA)of 1996. Although this act explicitly prohibits use of “full face photographic images and any comparable images” without consent from the patient or the patient’s representative, there is less restriction regarding the use of deidentified images.⁶ Some clinicians or researchers may consider using a black bar or a masking technique over the eyes or face, but this is not always a sufficient method of anonymizing an image.

One study investigating the different requirements listed by the top 20 dermatology journals (as determined by the Google Scholar h5-index) found that while 95% (19/20) of journals stated that written or signed consent or permission was a requirement for use of patient images, only 20% (4/20) instructed authors to inform the patient or the patient’s representative that images may become available on the internet.⁵ Once an article is accepted for publication by a medical journal, it eventually may be accessible online; however, patients may not be aware of this factor, which is particularly concerning for those with SOC due to the increased demand for diverse dermatologic resources and images as well as the highly digitalized manner in which we access and share media.

Furthermore, cultural and social factors exist that present challenges to informed decision-making during the consenting process for certain SOC populations such as a lack of trust in the medical and scientific research community, inadequate comprehension of the consent material, health illiteracy, language barriers, or use of complex terminology in consent documentation.^7,8 Studies also have shown that patients in ethnic minority groups have greater barriers to health literacy compared to other patient groups, and patients with limited health literacy are less likely to ask questions during their medical visits.^9,10 Therefore, when obtaining informed consent for images, it is important that measures are taken to ensure that the patient has full knowledge and understanding of what the consent covers, including the extent to which the images will be used and/or shared and whether the patient’s confidentiality and/or anonymity are at risk.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Encourage influential dermatology organizations such as the American Academy of Dermatology to establish standardized consenting procedures for image acquisition and use, including requirements to provide (a) written consent for all patient images and (b) specific details as to where and how the image may be used and/or shared.

2. Ensure that consent terminology is presented at a sixth-grade reading level or below, minimize the use of medical jargon and complex terms, and provide consent documentation in the patient’s preferred language.

3. Allow patients to take the consent document home so they can have additional time to comprehensively review the material or have it reviewed by family or friends.

4. Employ strategies such as teach-back methods and encourage questions to maximize the level of understanding during the consent process.

Clinical Image Storage

Clinical image storage procedures can have an impact on a patient’s health information remaining anonymous and confidential. In a survey evaluating medical photography use among 153 US board-certified dermatologists, 69.1% of respondents reported emailing or texting images between patients and colleagues. Additionally, 30.3% (46/152) reported having patient photographs stored on their personal phone at the time of the survey, and 39.1% (18/46) of those individuals had images that showed identifiable features, such as the patient’s face or a tattoo.¹¹

Although most providers state that their devices are password protected, it cannot be guaranteed that the device and consequently the images remain secure and inaccessible to unauthorized individuals. As sharing and viewing images continue to play an essential role in assessing disease state, progression, treatment response, and inclusion in research, we must establish and encourage clear guidelines for the storage and retention of such images.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Store clinical images exclusively on password-protected devices and in password-protected files.

2. Use work-related cameras or electronic devices rather than personal devices, unless the personal device is being used to upload directly into the patient’s medical record. In such cases, use a HIPAA-compliant electronic medical record mobile application that does not store images on the application or the device itself.

3. Avoid using text-messaging systems or unencrypted email to share identifying images without clear patient consent.

Clinical Image Use

Once a thorough consenting process has been completed, it is crucial that the use and distribution of the clinical image are in accordance with the terms specified in the original consent. With the current state of technologic advancement, widespread social media usage, and constant sharing of information, adherence to these terms can be challenging. For example, an image initially intended for use in an educational presentation at a professional conference can be shared on social media if an audience member captures a photo of it. In another example, a patient may consent to their image being shown on a dermatologic website but that image can be duplicated and shared on other unauthorized sites and locations. This situation can be particularly distressing to patients whose image may include all or most of their face, an intimate area, or other physical features that they did not wish to share widely.

Individuals identifying as Black/African American, Latino/Hispanic, or Asian have been shown to express less comfort with providing permission for images of a nonidentifiable sensitive area to be taken (or obtained) or for use for teaching irrespective of identifiability compared to their White counterparts,¹² which may be due to the aforementioned lack of trust in medical providers and the health care system in general, both of which may contribute to concerns with how a clinical image is used and/or shared. Although consent from a patient or the patient’s representative can be granted, we must ensure that the use of these images adheres to the patient’s initial agreement. Ultimately, medical providers, researchers, and other parties involved in acquiring or sharing patient images have both an ethical and legal responsibility to ensure that anonymity, privacy, and confidentiality are preserved to the greatest extent possible.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Display a message on websites containing patient images stating that the sharing of the images outside the established guidelines and intended use is prohibited.

2. Place a watermark on images to discourage unauthorized duplication.

3. Issue explicit instructions to audiences prohibiting the copying or reproducing of any patient images during teaching events or presentations.

Final Thoughts

The use of clinical images is an essential component of dermatologic care, education, and research. Due to the higher demand for diverse and representative images and the dearth of images in the medical literature, many SOC images have been widely disseminated and utilized by dermatologists, raising concerns of the adequacy of informed consent for the storage and use of such material. Therefore, dermatologists should implement streamlined guidelines and consent procedures to ensure a patient’s informed consent is provided with full knowledge of how and where their images might be used and shared. Additional efforts should be made to protect patients’ privacy and unauthorized use of their images. Furthermore, we encourage our leading dermatology organizations to develop expert consensus on best practices for appropriate clinical image consent, storage, and use.

Clinical images are integral to dermatologic care, research, and education. Studies have highlighted the underrepresentation of images of skin of color (SOC) in educational materials,¹ clinical trials,² and research publications.³ Recognition of this disparity has ignited a call to action by dermatologists and dermatologic organizations to address the gap by improving the collection and use of SOC images.⁴ It is critical to remind dermatologists of the importance of properly obtaining informed consent and ensuring images are not used without a patient’s permission, as images in journal articles, conference presentations, and educational materials can be widely distributed and shared. Herein, we summarize current practices of clinical image storage and make general recommendations on how dermatologists can better protect patient privacy. Certain cultural and social factors in patients with SOC should be considered when obtaining informed consent and collecting images.

Clinical Image Acquisition

Consenting procedures are crucial components of proper image usage. However, current consenting practices are inconsistent across various platforms, including academic journals, websites, printed text, social media, and educational presentations.⁵

Current regulations for use of patient health information in the United States are governed by the Health Insurance Portability and Accountability Act (HIPAA)of 1996. Although this act explicitly prohibits use of “full face photographic images and any comparable images” without consent from the patient or the patient’s representative, there is less restriction regarding the use of deidentified images.⁶ Some clinicians or researchers may consider using a black bar or a masking technique over the eyes or face, but this is not always a sufficient method of anonymizing an image.

One study investigating the different requirements listed by the top 20 dermatology journals (as determined by the Google Scholar h5-index) found that while 95% (19/20) of journals stated that written or signed consent or permission was a requirement for use of patient images, only 20% (4/20) instructed authors to inform the patient or the patient’s representative that images may become available on the internet.⁵ Once an article is accepted for publication by a medical journal, it eventually may be accessible online; however, patients may not be aware of this factor, which is particularly concerning for those with SOC due to the increased demand for diverse dermatologic resources and images as well as the highly digitalized manner in which we access and share media.

Furthermore, cultural and social factors exist that present challenges to informed decision-making during the consenting process for certain SOC populations such as a lack of trust in the medical and scientific research community, inadequate comprehension of the consent material, health illiteracy, language barriers, or use of complex terminology in consent documentation.^7,8 Studies also have shown that patients in ethnic minority groups have greater barriers to health literacy compared to other patient groups, and patients with limited health literacy are less likely to ask questions during their medical visits.^9,10 Therefore, when obtaining informed consent for images, it is important that measures are taken to ensure that the patient has full knowledge and understanding of what the consent covers, including the extent to which the images will be used and/or shared and whether the patient’s confidentiality and/or anonymity are at risk.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Encourage influential dermatology organizations such as the American Academy of Dermatology to establish standardized consenting procedures for image acquisition and use, including requirements to provide (a) written consent for all patient images and (b) specific details as to where and how the image may be used and/or shared.

2. Ensure that consent terminology is presented at a sixth-grade reading level or below, minimize the use of medical jargon and complex terms, and provide consent documentation in the patient’s preferred language.

3. Allow patients to take the consent document home so they can have additional time to comprehensively review the material or have it reviewed by family or friends.

4. Employ strategies such as teach-back methods and encourage questions to maximize the level of understanding during the consent process.

Clinical Image Storage

Clinical image storage procedures can have an impact on a patient’s health information remaining anonymous and confidential. In a survey evaluating medical photography use among 153 US board-certified dermatologists, 69.1% of respondents reported emailing or texting images between patients and colleagues. Additionally, 30.3% (46/152) reported having patient photographs stored on their personal phone at the time of the survey, and 39.1% (18/46) of those individuals had images that showed identifiable features, such as the patient’s face or a tattoo.¹¹

Although most providers state that their devices are password protected, it cannot be guaranteed that the device and consequently the images remain secure and inaccessible to unauthorized individuals. As sharing and viewing images continue to play an essential role in assessing disease state, progression, treatment response, and inclusion in research, we must establish and encourage clear guidelines for the storage and retention of such images.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Store clinical images exclusively on password-protected devices and in password-protected files.

2. Use work-related cameras or electronic devices rather than personal devices, unless the personal device is being used to upload directly into the patient’s medical record. In such cases, use a HIPAA-compliant electronic medical record mobile application that does not store images on the application or the device itself.

3. Avoid using text-messaging systems or unencrypted email to share identifying images without clear patient consent.

Clinical Image Use

Once a thorough consenting process has been completed, it is crucial that the use and distribution of the clinical image are in accordance with the terms specified in the original consent. With the current state of technologic advancement, widespread social media usage, and constant sharing of information, adherence to these terms can be challenging. For example, an image initially intended for use in an educational presentation at a professional conference can be shared on social media if an audience member captures a photo of it. In another example, a patient may consent to their image being shown on a dermatologic website but that image can be duplicated and shared on other unauthorized sites and locations. This situation can be particularly distressing to patients whose image may include all or most of their face, an intimate area, or other physical features that they did not wish to share widely.

Individuals identifying as Black/African American, Latino/Hispanic, or Asian have been shown to express less comfort with providing permission for images of a nonidentifiable sensitive area to be taken (or obtained) or for use for teaching irrespective of identifiability compared to their White counterparts,¹² which may be due to the aforementioned lack of trust in medical providers and the health care system in general, both of which may contribute to concerns with how a clinical image is used and/or shared. Although consent from a patient or the patient’s representative can be granted, we must ensure that the use of these images adheres to the patient’s initial agreement. Ultimately, medical providers, researchers, and other parties involved in acquiring or sharing patient images have both an ethical and legal responsibility to ensure that anonymity, privacy, and confidentiality are preserved to the greatest extent possible.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Display a message on websites containing patient images stating that the sharing of the images outside the established guidelines and intended use is prohibited.

2. Place a watermark on images to discourage unauthorized duplication.

3. Issue explicit instructions to audiences prohibiting the copying or reproducing of any patient images during teaching events or presentations.

Final Thoughts

The use of clinical images is an essential component of dermatologic care, education, and research. Due to the higher demand for diverse and representative images and the dearth of images in the medical literature, many SOC images have been widely disseminated and utilized by dermatologists, raising concerns of the adequacy of informed consent for the storage and use of such material. Therefore, dermatologists should implement streamlined guidelines and consent procedures to ensure a patient’s informed consent is provided with full knowledge of how and where their images might be used and shared. Additional efforts should be made to protect patients’ privacy and unauthorized use of their images. Furthermore, we encourage our leading dermatology organizations to develop expert consensus on best practices for appropriate clinical image consent, storage, and use.

Clinical images are integral to dermatologic care, research, and education. Studies have highlighted the underrepresentation of images of skin of color (SOC) in educational materials,¹ clinical trials,² and research publications.³ Recognition of this disparity has ignited a call to action by dermatologists and dermatologic organizations to address the gap by improving the collection and use of SOC images.⁴ It is critical to remind dermatologists of the importance of properly obtaining informed consent and ensuring images are not used without a patient’s permission, as images in journal articles, conference presentations, and educational materials can be widely distributed and shared. Herein, we summarize current practices of clinical image storage and make general recommendations on how dermatologists can better protect patient privacy. Certain cultural and social factors in patients with SOC should be considered when obtaining informed consent and collecting images.

Clinical Image Acquisition

Consenting procedures are crucial components of proper image usage. However, current consenting practices are inconsistent across various platforms, including academic journals, websites, printed text, social media, and educational presentations.⁵

Current regulations for use of patient health information in the United States are governed by the Health Insurance Portability and Accountability Act (HIPAA)of 1996. Although this act explicitly prohibits use of “full face photographic images and any comparable images” without consent from the patient or the patient’s representative, there is less restriction regarding the use of deidentified images.⁶ Some clinicians or researchers may consider using a black bar or a masking technique over the eyes or face, but this is not always a sufficient method of anonymizing an image.

One study investigating the different requirements listed by the top 20 dermatology journals (as determined by the Google Scholar h5-index) found that while 95% (19/20) of journals stated that written or signed consent or permission was a requirement for use of patient images, only 20% (4/20) instructed authors to inform the patient or the patient’s representative that images may become available on the internet.⁵ Once an article is accepted for publication by a medical journal, it eventually may be accessible online; however, patients may not be aware of this factor, which is particularly concerning for those with SOC due to the increased demand for diverse dermatologic resources and images as well as the highly digitalized manner in which we access and share media.

Furthermore, cultural and social factors exist that present challenges to informed decision-making during the consenting process for certain SOC populations such as a lack of trust in the medical and scientific research community, inadequate comprehension of the consent material, health illiteracy, language barriers, or use of complex terminology in consent documentation.^7,8 Studies also have shown that patients in ethnic minority groups have greater barriers to health literacy compared to other patient groups, and patients with limited health literacy are less likely to ask questions during their medical visits.^9,10 Therefore, when obtaining informed consent for images, it is important that measures are taken to ensure that the patient has full knowledge and understanding of what the consent covers, including the extent to which the images will be used and/or shared and whether the patient’s confidentiality and/or anonymity are at risk.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Encourage influential dermatology organizations such as the American Academy of Dermatology to establish standardized consenting procedures for image acquisition and use, including requirements to provide (a) written consent for all patient images and (b) specific details as to where and how the image may be used and/or shared.

2. Ensure that consent terminology is presented at a sixth-grade reading level or below, minimize the use of medical jargon and complex terms, and provide consent documentation in the patient’s preferred language.

3. Allow patients to take the consent document home so they can have additional time to comprehensively review the material or have it reviewed by family or friends.

4. Employ strategies such as teach-back methods and encourage questions to maximize the level of understanding during the consent process.

Clinical Image Storage

Clinical image storage procedures can have an impact on a patient’s health information remaining anonymous and confidential. In a survey evaluating medical photography use among 153 US board-certified dermatologists, 69.1% of respondents reported emailing or texting images between patients and colleagues. Additionally, 30.3% (46/152) reported having patient photographs stored on their personal phone at the time of the survey, and 39.1% (18/46) of those individuals had images that showed identifiable features, such as the patient’s face or a tattoo.¹¹

Although most providers state that their devices are password protected, it cannot be guaranteed that the device and consequently the images remain secure and inaccessible to unauthorized individuals. As sharing and viewing images continue to play an essential role in assessing disease state, progression, treatment response, and inclusion in research, we must establish and encourage clear guidelines for the storage and retention of such images.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Store clinical images exclusively on password-protected devices and in password-protected files.

2. Use work-related cameras or electronic devices rather than personal devices, unless the personal device is being used to upload directly into the patient’s medical record. In such cases, use a HIPAA-compliant electronic medical record mobile application that does not store images on the application or the device itself.

3. Avoid using text-messaging systems or unencrypted email to share identifying images without clear patient consent.

Clinical Image Use

Once a thorough consenting process has been completed, it is crucial that the use and distribution of the clinical image are in accordance with the terms specified in the original consent. With the current state of technologic advancement, widespread social media usage, and constant sharing of information, adherence to these terms can be challenging. For example, an image initially intended for use in an educational presentation at a professional conference can be shared on social media if an audience member captures a photo of it. In another example, a patient may consent to their image being shown on a dermatologic website but that image can be duplicated and shared on other unauthorized sites and locations. This situation can be particularly distressing to patients whose image may include all or most of their face, an intimate area, or other physical features that they did not wish to share widely.

Individuals identifying as Black/African American, Latino/Hispanic, or Asian have been shown to express less comfort with providing permission for images of a nonidentifiable sensitive area to be taken (or obtained) or for use for teaching irrespective of identifiability compared to their White counterparts,¹² which may be due to the aforementioned lack of trust in medical providers and the health care system in general, both of which may contribute to concerns with how a clinical image is used and/or shared. Although consent from a patient or the patient’s representative can be granted, we must ensure that the use of these images adheres to the patient’s initial agreement. Ultimately, medical providers, researchers, and other parties involved in acquiring or sharing patient images have both an ethical and legal responsibility to ensure that anonymity, privacy, and confidentiality are preserved to the greatest extent possible.

Recommendations—We propose that dermatologists should follow these recommendations:

1. Display a message on websites containing patient images stating that the sharing of the images outside the established guidelines and intended use is prohibited.

2. Place a watermark on images to discourage unauthorized duplication.

3. Issue explicit instructions to audiences prohibiting the copying or reproducing of any patient images during teaching events or presentations.

Final Thoughts

The use of clinical images is an essential component of dermatologic care, education, and research. Due to the higher demand for diverse and representative images and the dearth of images in the medical literature, many SOC images have been widely disseminated and utilized by dermatologists, raising concerns of the adequacy of informed consent for the storage and use of such material. Therefore, dermatologists should implement streamlined guidelines and consent procedures to ensure a patient’s informed consent is provided with full knowledge of how and where their images might be used and shared. Additional efforts should be made to protect patients’ privacy and unauthorized use of their images. Furthermore, we encourage our leading dermatology organizations to develop expert consensus on best practices for appropriate clinical image consent, storage, and use.

Practice Gap

Lichen planus (LP)—a chronic inflammatory disorder affecting the nails—is prevalent in 10% to 15% of patients and is more common in the fingernails than toenails. Clinical manifestation includes longitudinal ridges, nail plate atrophy, and splitting, which all contribute to cosmetic disfigurement and difficulty with functionality. Quality of life and daily activities may be impacted profoundly.¹ First-line therapies include intralesional and systemic corticosteroids; however, efficacy is limited and recurrence is common.^1,2 Lichen planus is one of the few conditions that may cause permanent and debilitating nail loss.

Tools

A resin nail can be used to improve cosmetic appearance and functionality in patients with recalcitrant nail LP. The composite resin creates a flexible nonporous nail and allows the underlying natural nail to grow. Application of resin nails has been used for toenail onychodystrophies to improve cosmesis and functionality but has not been reported for fingernails. The resin typically lasts 6 to 8 weeks on toenails.

The Technique

Application of a resin nail involves several steps (see video online). First, the affected nail should be debrided and a bonding agent applied. Next, multiple layers of resin are applied until the patient’s desired thickness is achieved (typically 2 layers), followed by a sealing agent. Finally, the nail is cured with UV light. We recommend applying sunscreen to the hand(s) prior to curing with UV light. The liquid resin allows the nail to be customized to the patient’s desired length and shape. The overall procedure takes approximately 20 minutes for a single nail.

We applied resin nail to the thumbnail of a 46-year-old woman with recalcitrant isolated nail LP of 7 years’ duration (Figure). She previously had difficulties performing everyday activities, and the resin improved her functionality. She also was pleased with the cosmetic appearance. After 2 weeks, the resin started falling off with corresponding natural nail growth. The patient denied any adverse events.

Practice Implications

Resin nail application may serve as a temporary solution to improve cosmesis and functionality in patients with recalcitrant nail LP. As shown in our patient, the resin may fall off faster on the fingernails than the toenails, likely because of the faster growth rate of fingernails and more frequent exposure from daily activities. Further studies of resin nail application for the fingernails are needed to establish duration in patients with varying levels of activity (eg, washing dishes, woodworking).

Because the resin nail may be removed easily at any time, resin nail application does not interfere with treatments such as intralesional steroid injections. For patients using a topical medication regimen, the resin nail may be applied slightly distal to the cuticle so that the medication can still be applied by the proximal nail fold of the underlying natural nail.

The resin nail should be kept short and removed after 2 to 4 weeks for the fingernails and 6 to 8 weeks for the toenails to examine the underlying natural nail. Patients may go about their daily activities with the resin nail, including applying nail polish to the resin nail, bathing, and swimming. Resin nail application may complement medical treatments and improve quality of life for patients with nail LP.

Practice Gap

Lichen planus (LP)—a chronic inflammatory disorder affecting the nails—is prevalent in 10% to 15% of patients and is more common in the fingernails than toenails. Clinical manifestation includes longitudinal ridges, nail plate atrophy, and splitting, which all contribute to cosmetic disfigurement and difficulty with functionality. Quality of life and daily activities may be impacted profoundly.¹ First-line therapies include intralesional and systemic corticosteroids; however, efficacy is limited and recurrence is common.^1,2 Lichen planus is one of the few conditions that may cause permanent and debilitating nail loss.

Tools

A resin nail can be used to improve cosmetic appearance and functionality in patients with recalcitrant nail LP. The composite resin creates a flexible nonporous nail and allows the underlying natural nail to grow. Application of resin nails has been used for toenail onychodystrophies to improve cosmesis and functionality but has not been reported for fingernails. The resin typically lasts 6 to 8 weeks on toenails.

The Technique

Application of a resin nail involves several steps (see video online). First, the affected nail should be debrided and a bonding agent applied. Next, multiple layers of resin are applied until the patient’s desired thickness is achieved (typically 2 layers), followed by a sealing agent. Finally, the nail is cured with UV light. We recommend applying sunscreen to the hand(s) prior to curing with UV light. The liquid resin allows the nail to be customized to the patient’s desired length and shape. The overall procedure takes approximately 20 minutes for a single nail.

We applied resin nail to the thumbnail of a 46-year-old woman with recalcitrant isolated nail LP of 7 years’ duration (Figure). She previously had difficulties performing everyday activities, and the resin improved her functionality. She also was pleased with the cosmetic appearance. After 2 weeks, the resin started falling off with corresponding natural nail growth. The patient denied any adverse events.

Practice Implications

Resin nail application may serve as a temporary solution to improve cosmesis and functionality in patients with recalcitrant nail LP. As shown in our patient, the resin may fall off faster on the fingernails than the toenails, likely because of the faster growth rate of fingernails and more frequent exposure from daily activities. Further studies of resin nail application for the fingernails are needed to establish duration in patients with varying levels of activity (eg, washing dishes, woodworking).

Because the resin nail may be removed easily at any time, resin nail application does not interfere with treatments such as intralesional steroid injections. For patients using a topical medication regimen, the resin nail may be applied slightly distal to the cuticle so that the medication can still be applied by the proximal nail fold of the underlying natural nail.

The resin nail should be kept short and removed after 2 to 4 weeks for the fingernails and 6 to 8 weeks for the toenails to examine the underlying natural nail. Patients may go about their daily activities with the resin nail, including applying nail polish to the resin nail, bathing, and swimming. Resin nail application may complement medical treatments and improve quality of life for patients with nail LP.

Practice Gap

Lichen planus (LP)—a chronic inflammatory disorder affecting the nails—is prevalent in 10% to 15% of patients and is more common in the fingernails than toenails. Clinical manifestation includes longitudinal ridges, nail plate atrophy, and splitting, which all contribute to cosmetic disfigurement and difficulty with functionality. Quality of life and daily activities may be impacted profoundly.¹ First-line therapies include intralesional and systemic corticosteroids; however, efficacy is limited and recurrence is common.^1,2 Lichen planus is one of the few conditions that may cause permanent and debilitating nail loss.

Tools

A resin nail can be used to improve cosmetic appearance and functionality in patients with recalcitrant nail LP. The composite resin creates a flexible nonporous nail and allows the underlying natural nail to grow. Application of resin nails has been used for toenail onychodystrophies to improve cosmesis and functionality but has not been reported for fingernails. The resin typically lasts 6 to 8 weeks on toenails.

The Technique

Application of a resin nail involves several steps (see video online). First, the affected nail should be debrided and a bonding agent applied. Next, multiple layers of resin are applied until the patient’s desired thickness is achieved (typically 2 layers), followed by a sealing agent. Finally, the nail is cured with UV light. We recommend applying sunscreen to the hand(s) prior to curing with UV light. The liquid resin allows the nail to be customized to the patient’s desired length and shape. The overall procedure takes approximately 20 minutes for a single nail.

We applied resin nail to the thumbnail of a 46-year-old woman with recalcitrant isolated nail LP of 7 years’ duration (Figure). She previously had difficulties performing everyday activities, and the resin improved her functionality. She also was pleased with the cosmetic appearance. After 2 weeks, the resin started falling off with corresponding natural nail growth. The patient denied any adverse events.

Practice Implications

Resin nail application may serve as a temporary solution to improve cosmesis and functionality in patients with recalcitrant nail LP. As shown in our patient, the resin may fall off faster on the fingernails than the toenails, likely because of the faster growth rate of fingernails and more frequent exposure from daily activities. Further studies of resin nail application for the fingernails are needed to establish duration in patients with varying levels of activity (eg, washing dishes, woodworking).

Because the resin nail may be removed easily at any time, resin nail application does not interfere with treatments such as intralesional steroid injections. For patients using a topical medication regimen, the resin nail may be applied slightly distal to the cuticle so that the medication can still be applied by the proximal nail fold of the underlying natural nail.

The resin nail should be kept short and removed after 2 to 4 weeks for the fingernails and 6 to 8 weeks for the toenails to examine the underlying natural nail. Patients may go about their daily activities with the resin nail, including applying nail polish to the resin nail, bathing, and swimming. Resin nail application may complement medical treatments and improve quality of life for patients with nail LP.

Alopecia areata (AA) affects 4.5 million individuals in the United States, with 66% younger than 30 years.^1,2 Inflammation causes hair loss in well-circumscribed, nonscarring patches on the body with a predilection for the scalp.^3-6 The disease can devastate a patient’s self-esteem, in turn reducing quality of life.^1,7 Alopecia areata is an autoimmune T-cell–mediated disease in which hair follicles lose their immune privilege.^8-10 Several specific mechanisms in the cytokine interactions between T cells and the hair follicle have been discovered, revealing the Janus kinase–signal transducer and activator of transcription (JAK-STAT) pathway as pivotal in the pathogenesis of the disease and leading to the use of JAK inhibitors for treatment.¹¹

There is no cure for AA, and the condition is managed with prolonged medical treatments and cosmetic therapies.² Although some patients may be able to manage the annual cost, the cumulative cost of AA treatment can be burdensome.¹² This cumulative cost may increase if newer, potentially expensive treatments become the standard of care. Patients with AA report dipping into their savings (41.3%) and cutting back on food or clothing expenses (33.9%) to account for the cost of alopecia treatment. Although prior estimates of the annual out-of-pocket cost of AA treatments range from $1354 to $2685, the cost burden of individual therapies is poorly understood.^12-14

Patients who must juggle expensive medical bills with basic living expenses may be lost to follow-up or fall into treatment nonadherence.¹⁵ Other patients’ out-of-pocket costs may be manageable, but the costs to the health care system may compromise care in other ways. We conducted a literature review of the recommended therapies for AA based on American Academy of Dermatology (AAD) guidelines to identify the costs of alopecia treatment and consolidate the available data for the practicing dermatologist.

Methods

We conducted a PubMed search of articles indexed for MEDLINE through September 15, 2022, using the terms alopecia and cost plus one of the treatments (n=21) identified by the AAD² for the treatment of AA (Figure). The reference lists of included articles were reviewed to identify other potentially relevant studies. Forty-five articles were identified.

Given the dearth of cost research in alopecia and the paucity of large prospective studies, we excluded articles that were not available in their full-text form or were not in English (n=3), articles whose primary study topic was not AA or an expert-approved alopecia treatment (n=15), and articles with no concrete cost data (n=17), which yielded 10 relevant articles that we studied using qualitative analysis.

Due to substantial differences in study methods and outcome measures, we did not compare the costs of alopecia among studies and did not perform statistical analysis. The quality of each study was investigated and assigned a level of evidence per the 2009 criteria from the Centre for Evidence-Based Medicine.¹⁶

All cost data were converted into US dollars ($) using the conversion rate from the time of the original article’s publication.

Results

Total and Out-of-pocket Costs of AA—Li et al¹³ studied out-of-pocket health care costs for AA patients (N=675). Of these participants, 56.9% said their AA was moderately to seriously financially burdensome, and 41.3% reported using their savings to manage these expenses. Participants reported median out-of-pocket spending of $1354 (interquartile range, $537–$3300) annually. The most common categories of expenses were hair appointments (81.8%) and vitamins/supplements (67.7%).¹³

Mesinkovska et al¹⁴ studied the qualitative and quantitative financial burdens of moderate to severe AA (N=216). Fifty-seven percent of patients reported the financial impact of AA as moderately to severely burdensome with a willingness to borrow money or use savings to cover out-of-pocket costs. Patients without insurance cited cost as a major barrier to obtaining reatment. In addition to direct treatment-related expenses, AA patients spent a mean of $1961 per year on therapy to cope with the disease’s psychological burden. Lost work hours represented another source of financial burden; 61% of patients were employed, and 45% of them reported missing time from their job because of AA.¹⁴

Mostaghimi et al¹² studied health care resource utilization and all-cause direct health care costs in privately insured AA patients with or without alopecia totalis (AT) or alopecia universalis (AU)(n=14,972) matched with non-AA controls (n=44,916)(1:3 ratio). Mean total all-cause medical and pharmacy costs were higher in both AA groups compared with controls (AT/AU, $18,988 vs $11,030; non-AT/AU, $13,686 vs $9336; P<.001 for both). Out-of-pocket costs were higher for AA vs controls (AT/AU, $2685 vs $1457; non-AT/AU, $2223 vs $1341; P<.001 for both). Medical costs in the AT/AU and non-AT/AU groups largely were driven by outpatient costs (AT/AU, $10,277 vs $5713; non-AT/AU, $8078 vs $4672; P<.001 for both).¹²

Costs of Concealment—When studying the out-of-pocket costs of AA (N=675), Li et al¹³ discovered that the median yearly spending was highest on headwear or cosmetic items such as hats, wigs, and makeup ($450; interquartile range, $50–$1500). Mesinkovska et al¹⁴ reported that 49% of patients had insurance that covered AA treatment. However, 75% of patients reported that their insurance would not cover costs of concealment (eg, weave, wig, hair piece). Patients (N=112) spent a mean of $2211 per year and 10.3 hours per week on concealment.¹⁴

Minoxidil—Minoxidil solution is available over-the-counter, and its ease of access makes it a popular treatment for AA.¹⁷ Because manufacturers can sell directly to the public, minoxidil is marketed with bold claims and convincing packaging. Shrank¹⁸ noted that the product can take 4 months to work, meaning customers must incur a substantial cost burden before realizing the treatment’s benefit, which is not always obvious when purchasing minoxidil products, leaving customers—who were marketed a miracle drug—disappointed. Per Shrank,¹⁸ patients who did not experience hair regrowth after 4 months were advised to continue treatment for a year, leading them to spend hundreds of dollars for uncertain results. Those who did experience hair regrowth were advised to continue using the product twice daily 7 days per week indefinitely.¹⁸

Wehner et al¹⁹ studied the association between gender and drug cost for over-the-counter minoxidil. The price that women paid for 2% regular-strength minoxidil solutions was similar to the price that men paid for 5% extra-strength minoxidil solutions (women’s 2%, $7.63/30 mL; men’s 5%, $7.61/30 mL; P=.67). Minoxidil 5% foams with identical ingredients were priced significantly more per volume of the same product when sold as a product directed at women vs a product directed at men (men’s 5%, $8.05/30 mL; women’s 5%, $11.27/30 mL; P<.001).¹⁹

Beach²⁰ compared the cost of oral minoxidil to topical minoxidil. At $28.60 for a 3-month supply, oral minoxidil demonstrated cost savings compared to topical minoxidil ($48.30).²⁰

Diphencyprone—Bhat et al²¹ studied the cost-efficiency of diphencyprone (DPC) in patients with AA resistant to at least 2 conventional treatments (N=29). After initial sensitization with 2% DPC, patients received weekly or fortnightly treatments. Most of the annual cost burden of DPC treatment was due to staff time and overhead rather than the cost of the DPC itself: $258 for the DPC, $978 in staff time and overhead for the department, and $1233 directly charged to the patient.²¹

Lekhavat et al²² studied the economic impact of home-use vs office-use DPC in extensive AA (N=82). Both groups received weekly treatments in the hospital until DPC concentrations had been adjusted. Afterward, the home group was given training on self-applying DPC at home. The home group had monthly office visits for DPC concentration evaluation and refills, while the office group had weekly appointments for DPC treatment at the hospital. Calculated costs included those to the health care provider (ie, material, labor, capital costs) and the patient’s final out-of-pocket expense. The total cost to the health care provider was higher for the office group than the home group at 48 weeks (office, $683.52; home, $303.67; P<.001). Median out-of-pocket costs did not vary significantly between groups, which may have been due to small sample size affecting the range (office, $418.07; home, $189.69; P=.101). There was no significant difference between groups in the proportion of patients who responded favorably to the DPC.²²

JAK Inhibitors—Chen et al²³ studied the efficacy of low-dose (5 mg) tofacitinib to treat severe AA (N=6). Compared to prior studies,^24-27 this analysis reported the efficacy of low-dose tofacitinib was not inferior to higher doses (10–20 mg), and low-dose tofacitinib reduced treatment costs by more than 50%.²³

Per the GlobalData Healthcare database, the estimated annual cost of therapy for JAK inhibitors following US Food and Drug Administration approval was $50,000. At the time of their reporting, the next most expensive immunomodulatory drug for AA was cyclosporine, with an annual cost of therapy of $1400.²⁸ Dillon²⁹ reviewed the use of JAK inhibitors for the treatment of AA. The cost estimates by Dillon²⁹ prior to FDA approval aligned with the pricing of Eli Lilly and Company for the now-approved JAK inhibitor baricitinib.³⁰ The list price of baricitinib is $2739.99 for a 30-day supply of 2-mg tablets or $5479.98 for a 30-day supply of 4-mg tablets. This amounts to $32,879.88 for an annual supply of 2-mg tablets and $65,759.76 for an annual supply for 4-mg tablets, though the out-of-pocket costs will vary.³⁰

Comment

We reviewed the global and treatment-specific costs of AA, consolidating the available data for the practicing dermatologist. Ten studies of approximately 16,000 patients with AA across a range of levels of evidence (1a to 4) were included (Table). Three of 10 articles studied global costs of AA, 1 studied costs of concealment, 3 studied costs of minoxidil, 2 studied costs of DPC, and 2 studied costs of JAK inhibitors. Only 2 studies achieved level of evidence 1a: the first assessed the economic impact of home-use vs office-use DPC,²² and the second researched the efficacy and outcomes of JAK inhibitors.²⁹

Hair-loss treatments and concealment techniques cost the average patient thousands of dollars. Spending was highest on headwear or cosmetic items, which were rarely covered by insurance.¹³ Psychosocial sequelae further increased cost via therapy charges and lost time at work.¹⁴ Patients with AA had greater all-cause medical costs than those without AA, with most of the cost driven by outpatient visits. Patients with AA also paid nearly twice as much as non-AA patients on out-of-pocket health care expenses.¹⁴ Despite the high costs and limited efficacy of many AA therapies, patients reported willingness to incur debt or use savings to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress.¹³

Minoxidil solution does not require physician office visits and is available over-the-counter.¹⁷ Despite identical ingredients, minoxidil is priced more per volume when marketed to women compared with men, which reflects the larger issue of gender-based pricing that does not exist for other AAD-approved alopecia therapies but may exist for cosmetic treatments and nonapproved therapies (eg, vitamins/supplements) that are popular in the treatment of AA.¹⁹ Oral minoxidil was more cost-effective than the topical form, and gender-based pricing was a nonissue.²⁰ However, oral minoxidil requires a prescription, mandating patients incur the cost of an office visit. Patients should be wary of gender- or marketing-related surcharges for minoxidil solutions, and oral minoxidil may be a cost-effective choice.

Diphencyprone is a relatively affordable drug for AA, but the regular office visits traditionally required for its administration increase associated cost.²¹ Self-administration of DPC at home was more cost- and time-effective than in-office DPC administration and did not decrease efficacy. A regimen combining office visits for initial DPC titration, at-home DPC administration, and periodic office follow-up could minimize costs while preserving outcomes and safety.²²

Janus kinase inhibitors are cutting-edge and expensive therapies for AA. The annual cost of these medications poses a tremendous burden on the payer (list price of annual supply ritlecitinib is $49,000),³¹ be that the patient or the insurance company. Low-dose tofacitinib may be similarly efficacious and could substantially reduce treatment costs.²³ The true utility of these medications, specifically considering their steep costs, remains to be determined.

Conclusion

Alopecia areata poses a substantial and recurring cost burden on patients that is multifactorial including treatment, office visits, concealment, alternative therapies, psychosocial costs, and missed time at work. Although several treatment options exist, none of them are definitive. Oral minoxidil and at-home DPC administration can be cost-effective, though the cumulative cost is still high. The cost utility of JAK inhibitors remains unclear. When JAK inhibitors are prescribed, low-dose therapy may be used as maintenance to curb treatment costs. Concealment and therapy costs pose an additional, largely out-of-pocket financial burden. Despite the limited efficacy of many AA therapies, patients incur substantial expenses to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress. There are no head-to-head studies comparing the cost-effectiveness of the different AA therapies; thus, it is unclear if one treatment is most efficacious. This topic remains an avenue for future investigation. Much of the cost burden of AA treatment falls directly on patients. Increasing coverage of AA-associated expenses, such as minoxidil therapy or wigs, could decrease the cost burden on patients. Providers also can inform patients about cost-saving tactics, such as purchasing minoxidil based on concentration and vehicle rather than marketing directed at men vs women. Finally, some patients may have insurance plans that at least partially cover the costs of wigs but may not be aware of this benefit. Querying a patient’s insurance provider can further minimize costs.

Alopecia areata (AA) affects 4.5 million individuals in the United States, with 66% younger than 30 years.^1,2 Inflammation causes hair loss in well-circumscribed, nonscarring patches on the body with a predilection for the scalp.^3-6 The disease can devastate a patient’s self-esteem, in turn reducing quality of life.^1,7 Alopecia areata is an autoimmune T-cell–mediated disease in which hair follicles lose their immune privilege.^8-10 Several specific mechanisms in the cytokine interactions between T cells and the hair follicle have been discovered, revealing the Janus kinase–signal transducer and activator of transcription (JAK-STAT) pathway as pivotal in the pathogenesis of the disease and leading to the use of JAK inhibitors for treatment.¹¹

There is no cure for AA, and the condition is managed with prolonged medical treatments and cosmetic therapies.² Although some patients may be able to manage the annual cost, the cumulative cost of AA treatment can be burdensome.¹² This cumulative cost may increase if newer, potentially expensive treatments become the standard of care. Patients with AA report dipping into their savings (41.3%) and cutting back on food or clothing expenses (33.9%) to account for the cost of alopecia treatment. Although prior estimates of the annual out-of-pocket cost of AA treatments range from $1354 to $2685, the cost burden of individual therapies is poorly understood.^12-14

Patients who must juggle expensive medical bills with basic living expenses may be lost to follow-up or fall into treatment nonadherence.¹⁵ Other patients’ out-of-pocket costs may be manageable, but the costs to the health care system may compromise care in other ways. We conducted a literature review of the recommended therapies for AA based on American Academy of Dermatology (AAD) guidelines to identify the costs of alopecia treatment and consolidate the available data for the practicing dermatologist.

Methods

We conducted a PubMed search of articles indexed for MEDLINE through September 15, 2022, using the terms alopecia and cost plus one of the treatments (n=21) identified by the AAD² for the treatment of AA (Figure). The reference lists of included articles were reviewed to identify other potentially relevant studies. Forty-five articles were identified.

Given the dearth of cost research in alopecia and the paucity of large prospective studies, we excluded articles that were not available in their full-text form or were not in English (n=3), articles whose primary study topic was not AA or an expert-approved alopecia treatment (n=15), and articles with no concrete cost data (n=17), which yielded 10 relevant articles that we studied using qualitative analysis.

Due to substantial differences in study methods and outcome measures, we did not compare the costs of alopecia among studies and did not perform statistical analysis. The quality of each study was investigated and assigned a level of evidence per the 2009 criteria from the Centre for Evidence-Based Medicine.¹⁶

All cost data were converted into US dollars ($) using the conversion rate from the time of the original article’s publication.

Results

Total and Out-of-pocket Costs of AA—Li et al¹³ studied out-of-pocket health care costs for AA patients (N=675). Of these participants, 56.9% said their AA was moderately to seriously financially burdensome, and 41.3% reported using their savings to manage these expenses. Participants reported median out-of-pocket spending of $1354 (interquartile range, $537–$3300) annually. The most common categories of expenses were hair appointments (81.8%) and vitamins/supplements (67.7%).¹³

Mesinkovska et al¹⁴ studied the qualitative and quantitative financial burdens of moderate to severe AA (N=216). Fifty-seven percent of patients reported the financial impact of AA as moderately to severely burdensome with a willingness to borrow money or use savings to cover out-of-pocket costs. Patients without insurance cited cost as a major barrier to obtaining reatment. In addition to direct treatment-related expenses, AA patients spent a mean of $1961 per year on therapy to cope with the disease’s psychological burden. Lost work hours represented another source of financial burden; 61% of patients were employed, and 45% of them reported missing time from their job because of AA.¹⁴

Mostaghimi et al¹² studied health care resource utilization and all-cause direct health care costs in privately insured AA patients with or without alopecia totalis (AT) or alopecia universalis (AU)(n=14,972) matched with non-AA controls (n=44,916)(1:3 ratio). Mean total all-cause medical and pharmacy costs were higher in both AA groups compared with controls (AT/AU, $18,988 vs $11,030; non-AT/AU, $13,686 vs $9336; P<.001 for both). Out-of-pocket costs were higher for AA vs controls (AT/AU, $2685 vs $1457; non-AT/AU, $2223 vs $1341; P<.001 for both). Medical costs in the AT/AU and non-AT/AU groups largely were driven by outpatient costs (AT/AU, $10,277 vs $5713; non-AT/AU, $8078 vs $4672; P<.001 for both).¹²

Costs of Concealment—When studying the out-of-pocket costs of AA (N=675), Li et al¹³ discovered that the median yearly spending was highest on headwear or cosmetic items such as hats, wigs, and makeup ($450; interquartile range, $50–$1500). Mesinkovska et al¹⁴ reported that 49% of patients had insurance that covered AA treatment. However, 75% of patients reported that their insurance would not cover costs of concealment (eg, weave, wig, hair piece). Patients (N=112) spent a mean of $2211 per year and 10.3 hours per week on concealment.¹⁴

Minoxidil—Minoxidil solution is available over-the-counter, and its ease of access makes it a popular treatment for AA.¹⁷ Because manufacturers can sell directly to the public, minoxidil is marketed with bold claims and convincing packaging. Shrank¹⁸ noted that the product can take 4 months to work, meaning customers must incur a substantial cost burden before realizing the treatment’s benefit, which is not always obvious when purchasing minoxidil products, leaving customers—who were marketed a miracle drug—disappointed. Per Shrank,¹⁸ patients who did not experience hair regrowth after 4 months were advised to continue treatment for a year, leading them to spend hundreds of dollars for uncertain results. Those who did experience hair regrowth were advised to continue using the product twice daily 7 days per week indefinitely.¹⁸

Wehner et al¹⁹ studied the association between gender and drug cost for over-the-counter minoxidil. The price that women paid for 2% regular-strength minoxidil solutions was similar to the price that men paid for 5% extra-strength minoxidil solutions (women’s 2%, $7.63/30 mL; men’s 5%, $7.61/30 mL; P=.67). Minoxidil 5% foams with identical ingredients were priced significantly more per volume of the same product when sold as a product directed at women vs a product directed at men (men’s 5%, $8.05/30 mL; women’s 5%, $11.27/30 mL; P<.001).¹⁹

Beach²⁰ compared the cost of oral minoxidil to topical minoxidil. At $28.60 for a 3-month supply, oral minoxidil demonstrated cost savings compared to topical minoxidil ($48.30).²⁰

Diphencyprone—Bhat et al²¹ studied the cost-efficiency of diphencyprone (DPC) in patients with AA resistant to at least 2 conventional treatments (N=29). After initial sensitization with 2% DPC, patients received weekly or fortnightly treatments. Most of the annual cost burden of DPC treatment was due to staff time and overhead rather than the cost of the DPC itself: $258 for the DPC, $978 in staff time and overhead for the department, and $1233 directly charged to the patient.²¹

Lekhavat et al²² studied the economic impact of home-use vs office-use DPC in extensive AA (N=82). Both groups received weekly treatments in the hospital until DPC concentrations had been adjusted. Afterward, the home group was given training on self-applying DPC at home. The home group had monthly office visits for DPC concentration evaluation and refills, while the office group had weekly appointments for DPC treatment at the hospital. Calculated costs included those to the health care provider (ie, material, labor, capital costs) and the patient’s final out-of-pocket expense. The total cost to the health care provider was higher for the office group than the home group at 48 weeks (office, $683.52; home, $303.67; P<.001). Median out-of-pocket costs did not vary significantly between groups, which may have been due to small sample size affecting the range (office, $418.07; home, $189.69; P=.101). There was no significant difference between groups in the proportion of patients who responded favorably to the DPC.²²

JAK Inhibitors—Chen et al²³ studied the efficacy of low-dose (5 mg) tofacitinib to treat severe AA (N=6). Compared to prior studies,^24-27 this analysis reported the efficacy of low-dose tofacitinib was not inferior to higher doses (10–20 mg), and low-dose tofacitinib reduced treatment costs by more than 50%.²³

Per the GlobalData Healthcare database, the estimated annual cost of therapy for JAK inhibitors following US Food and Drug Administration approval was $50,000. At the time of their reporting, the next most expensive immunomodulatory drug for AA was cyclosporine, with an annual cost of therapy of $1400.²⁸ Dillon²⁹ reviewed the use of JAK inhibitors for the treatment of AA. The cost estimates by Dillon²⁹ prior to FDA approval aligned with the pricing of Eli Lilly and Company for the now-approved JAK inhibitor baricitinib.³⁰ The list price of baricitinib is $2739.99 for a 30-day supply of 2-mg tablets or $5479.98 for a 30-day supply of 4-mg tablets. This amounts to $32,879.88 for an annual supply of 2-mg tablets and $65,759.76 for an annual supply for 4-mg tablets, though the out-of-pocket costs will vary.³⁰

Comment

We reviewed the global and treatment-specific costs of AA, consolidating the available data for the practicing dermatologist. Ten studies of approximately 16,000 patients with AA across a range of levels of evidence (1a to 4) were included (Table). Three of 10 articles studied global costs of AA, 1 studied costs of concealment, 3 studied costs of minoxidil, 2 studied costs of DPC, and 2 studied costs of JAK inhibitors. Only 2 studies achieved level of evidence 1a: the first assessed the economic impact of home-use vs office-use DPC,²² and the second researched the efficacy and outcomes of JAK inhibitors.²⁹

Hair-loss treatments and concealment techniques cost the average patient thousands of dollars. Spending was highest on headwear or cosmetic items, which were rarely covered by insurance.¹³ Psychosocial sequelae further increased cost via therapy charges and lost time at work.¹⁴ Patients with AA had greater all-cause medical costs than those without AA, with most of the cost driven by outpatient visits. Patients with AA also paid nearly twice as much as non-AA patients on out-of-pocket health care expenses.¹⁴ Despite the high costs and limited efficacy of many AA therapies, patients reported willingness to incur debt or use savings to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress.¹³

Minoxidil solution does not require physician office visits and is available over-the-counter.¹⁷ Despite identical ingredients, minoxidil is priced more per volume when marketed to women compared with men, which reflects the larger issue of gender-based pricing that does not exist for other AAD-approved alopecia therapies but may exist for cosmetic treatments and nonapproved therapies (eg, vitamins/supplements) that are popular in the treatment of AA.¹⁹ Oral minoxidil was more cost-effective than the topical form, and gender-based pricing was a nonissue.²⁰ However, oral minoxidil requires a prescription, mandating patients incur the cost of an office visit. Patients should be wary of gender- or marketing-related surcharges for minoxidil solutions, and oral minoxidil may be a cost-effective choice.

Diphencyprone is a relatively affordable drug for AA, but the regular office visits traditionally required for its administration increase associated cost.²¹ Self-administration of DPC at home was more cost- and time-effective than in-office DPC administration and did not decrease efficacy. A regimen combining office visits for initial DPC titration, at-home DPC administration, and periodic office follow-up could minimize costs while preserving outcomes and safety.²²

Janus kinase inhibitors are cutting-edge and expensive therapies for AA. The annual cost of these medications poses a tremendous burden on the payer (list price of annual supply ritlecitinib is $49,000),³¹ be that the patient or the insurance company. Low-dose tofacitinib may be similarly efficacious and could substantially reduce treatment costs.²³ The true utility of these medications, specifically considering their steep costs, remains to be determined.

Conclusion

Alopecia areata poses a substantial and recurring cost burden on patients that is multifactorial including treatment, office visits, concealment, alternative therapies, psychosocial costs, and missed time at work. Although several treatment options exist, none of them are definitive. Oral minoxidil and at-home DPC administration can be cost-effective, though the cumulative cost is still high. The cost utility of JAK inhibitors remains unclear. When JAK inhibitors are prescribed, low-dose therapy may be used as maintenance to curb treatment costs. Concealment and therapy costs pose an additional, largely out-of-pocket financial burden. Despite the limited efficacy of many AA therapies, patients incur substantial expenses to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress. There are no head-to-head studies comparing the cost-effectiveness of the different AA therapies; thus, it is unclear if one treatment is most efficacious. This topic remains an avenue for future investigation. Much of the cost burden of AA treatment falls directly on patients. Increasing coverage of AA-associated expenses, such as minoxidil therapy or wigs, could decrease the cost burden on patients. Providers also can inform patients about cost-saving tactics, such as purchasing minoxidil based on concentration and vehicle rather than marketing directed at men vs women. Finally, some patients may have insurance plans that at least partially cover the costs of wigs but may not be aware of this benefit. Querying a patient’s insurance provider can further minimize costs.

Alopecia areata (AA) affects 4.5 million individuals in the United States, with 66% younger than 30 years.^1,2 Inflammation causes hair loss in well-circumscribed, nonscarring patches on the body with a predilection for the scalp.^3-6 The disease can devastate a patient’s self-esteem, in turn reducing quality of life.^1,7 Alopecia areata is an autoimmune T-cell–mediated disease in which hair follicles lose their immune privilege.^8-10 Several specific mechanisms in the cytokine interactions between T cells and the hair follicle have been discovered, revealing the Janus kinase–signal transducer and activator of transcription (JAK-STAT) pathway as pivotal in the pathogenesis of the disease and leading to the use of JAK inhibitors for treatment.¹¹

There is no cure for AA, and the condition is managed with prolonged medical treatments and cosmetic therapies.² Although some patients may be able to manage the annual cost, the cumulative cost of AA treatment can be burdensome.¹² This cumulative cost may increase if newer, potentially expensive treatments become the standard of care. Patients with AA report dipping into their savings (41.3%) and cutting back on food or clothing expenses (33.9%) to account for the cost of alopecia treatment. Although prior estimates of the annual out-of-pocket cost of AA treatments range from $1354 to $2685, the cost burden of individual therapies is poorly understood.^12-14

Patients who must juggle expensive medical bills with basic living expenses may be lost to follow-up or fall into treatment nonadherence.¹⁵ Other patients’ out-of-pocket costs may be manageable, but the costs to the health care system may compromise care in other ways. We conducted a literature review of the recommended therapies for AA based on American Academy of Dermatology (AAD) guidelines to identify the costs of alopecia treatment and consolidate the available data for the practicing dermatologist.

Methods

We conducted a PubMed search of articles indexed for MEDLINE through September 15, 2022, using the terms alopecia and cost plus one of the treatments (n=21) identified by the AAD² for the treatment of AA (Figure). The reference lists of included articles were reviewed to identify other potentially relevant studies. Forty-five articles were identified.

Given the dearth of cost research in alopecia and the paucity of large prospective studies, we excluded articles that were not available in their full-text form or were not in English (n=3), articles whose primary study topic was not AA or an expert-approved alopecia treatment (n=15), and articles with no concrete cost data (n=17), which yielded 10 relevant articles that we studied using qualitative analysis.

Due to substantial differences in study methods and outcome measures, we did not compare the costs of alopecia among studies and did not perform statistical analysis. The quality of each study was investigated and assigned a level of evidence per the 2009 criteria from the Centre for Evidence-Based Medicine.¹⁶

All cost data were converted into US dollars ($) using the conversion rate from the time of the original article’s publication.

Results

Total and Out-of-pocket Costs of AA—Li et al¹³ studied out-of-pocket health care costs for AA patients (N=675). Of these participants, 56.9% said their AA was moderately to seriously financially burdensome, and 41.3% reported using their savings to manage these expenses. Participants reported median out-of-pocket spending of $1354 (interquartile range, $537–$3300) annually. The most common categories of expenses were hair appointments (81.8%) and vitamins/supplements (67.7%).¹³

Mesinkovska et al¹⁴ studied the qualitative and quantitative financial burdens of moderate to severe AA (N=216). Fifty-seven percent of patients reported the financial impact of AA as moderately to severely burdensome with a willingness to borrow money or use savings to cover out-of-pocket costs. Patients without insurance cited cost as a major barrier to obtaining reatment. In addition to direct treatment-related expenses, AA patients spent a mean of $1961 per year on therapy to cope with the disease’s psychological burden. Lost work hours represented another source of financial burden; 61% of patients were employed, and 45% of them reported missing time from their job because of AA.¹⁴

Mostaghimi et al¹² studied health care resource utilization and all-cause direct health care costs in privately insured AA patients with or without alopecia totalis (AT) or alopecia universalis (AU)(n=14,972) matched with non-AA controls (n=44,916)(1:3 ratio). Mean total all-cause medical and pharmacy costs were higher in both AA groups compared with controls (AT/AU, $18,988 vs $11,030; non-AT/AU, $13,686 vs $9336; P<.001 for both). Out-of-pocket costs were higher for AA vs controls (AT/AU, $2685 vs $1457; non-AT/AU, $2223 vs $1341; P<.001 for both). Medical costs in the AT/AU and non-AT/AU groups largely were driven by outpatient costs (AT/AU, $10,277 vs $5713; non-AT/AU, $8078 vs $4672; P<.001 for both).¹²

Costs of Concealment—When studying the out-of-pocket costs of AA (N=675), Li et al¹³ discovered that the median yearly spending was highest on headwear or cosmetic items such as hats, wigs, and makeup ($450; interquartile range, $50–$1500). Mesinkovska et al¹⁴ reported that 49% of patients had insurance that covered AA treatment. However, 75% of patients reported that their insurance would not cover costs of concealment (eg, weave, wig, hair piece). Patients (N=112) spent a mean of $2211 per year and 10.3 hours per week on concealment.¹⁴

Minoxidil—Minoxidil solution is available over-the-counter, and its ease of access makes it a popular treatment for AA.¹⁷ Because manufacturers can sell directly to the public, minoxidil is marketed with bold claims and convincing packaging. Shrank¹⁸ noted that the product can take 4 months to work, meaning customers must incur a substantial cost burden before realizing the treatment’s benefit, which is not always obvious when purchasing minoxidil products, leaving customers—who were marketed a miracle drug—disappointed. Per Shrank,¹⁸ patients who did not experience hair regrowth after 4 months were advised to continue treatment for a year, leading them to spend hundreds of dollars for uncertain results. Those who did experience hair regrowth were advised to continue using the product twice daily 7 days per week indefinitely.¹⁸

Wehner et al¹⁹ studied the association between gender and drug cost for over-the-counter minoxidil. The price that women paid for 2% regular-strength minoxidil solutions was similar to the price that men paid for 5% extra-strength minoxidil solutions (women’s 2%, $7.63/30 mL; men’s 5%, $7.61/30 mL; P=.67). Minoxidil 5% foams with identical ingredients were priced significantly more per volume of the same product when sold as a product directed at women vs a product directed at men (men’s 5%, $8.05/30 mL; women’s 5%, $11.27/30 mL; P<.001).¹⁹

Beach²⁰ compared the cost of oral minoxidil to topical minoxidil. At $28.60 for a 3-month supply, oral minoxidil demonstrated cost savings compared to topical minoxidil ($48.30).²⁰

Diphencyprone—Bhat et al²¹ studied the cost-efficiency of diphencyprone (DPC) in patients with AA resistant to at least 2 conventional treatments (N=29). After initial sensitization with 2% DPC, patients received weekly or fortnightly treatments. Most of the annual cost burden of DPC treatment was due to staff time and overhead rather than the cost of the DPC itself: $258 for the DPC, $978 in staff time and overhead for the department, and $1233 directly charged to the patient.²¹

Lekhavat et al²² studied the economic impact of home-use vs office-use DPC in extensive AA (N=82). Both groups received weekly treatments in the hospital until DPC concentrations had been adjusted. Afterward, the home group was given training on self-applying DPC at home. The home group had monthly office visits for DPC concentration evaluation and refills, while the office group had weekly appointments for DPC treatment at the hospital. Calculated costs included those to the health care provider (ie, material, labor, capital costs) and the patient’s final out-of-pocket expense. The total cost to the health care provider was higher for the office group than the home group at 48 weeks (office, $683.52; home, $303.67; P<.001). Median out-of-pocket costs did not vary significantly between groups, which may have been due to small sample size affecting the range (office, $418.07; home, $189.69; P=.101). There was no significant difference between groups in the proportion of patients who responded favorably to the DPC.²²

JAK Inhibitors—Chen et al²³ studied the efficacy of low-dose (5 mg) tofacitinib to treat severe AA (N=6). Compared to prior studies,^24-27 this analysis reported the efficacy of low-dose tofacitinib was not inferior to higher doses (10–20 mg), and low-dose tofacitinib reduced treatment costs by more than 50%.²³

Per the GlobalData Healthcare database, the estimated annual cost of therapy for JAK inhibitors following US Food and Drug Administration approval was $50,000. At the time of their reporting, the next most expensive immunomodulatory drug for AA was cyclosporine, with an annual cost of therapy of $1400.²⁸ Dillon²⁹ reviewed the use of JAK inhibitors for the treatment of AA. The cost estimates by Dillon²⁹ prior to FDA approval aligned with the pricing of Eli Lilly and Company for the now-approved JAK inhibitor baricitinib.³⁰ The list price of baricitinib is $2739.99 for a 30-day supply of 2-mg tablets or $5479.98 for a 30-day supply of 4-mg tablets. This amounts to $32,879.88 for an annual supply of 2-mg tablets and $65,759.76 for an annual supply for 4-mg tablets, though the out-of-pocket costs will vary.³⁰

Comment

We reviewed the global and treatment-specific costs of AA, consolidating the available data for the practicing dermatologist. Ten studies of approximately 16,000 patients with AA across a range of levels of evidence (1a to 4) were included (Table). Three of 10 articles studied global costs of AA, 1 studied costs of concealment, 3 studied costs of minoxidil, 2 studied costs of DPC, and 2 studied costs of JAK inhibitors. Only 2 studies achieved level of evidence 1a: the first assessed the economic impact of home-use vs office-use DPC,²² and the second researched the efficacy and outcomes of JAK inhibitors.²⁹

Hair-loss treatments and concealment techniques cost the average patient thousands of dollars. Spending was highest on headwear or cosmetic items, which were rarely covered by insurance.¹³ Psychosocial sequelae further increased cost via therapy charges and lost time at work.¹⁴ Patients with AA had greater all-cause medical costs than those without AA, with most of the cost driven by outpatient visits. Patients with AA also paid nearly twice as much as non-AA patients on out-of-pocket health care expenses.¹⁴ Despite the high costs and limited efficacy of many AA therapies, patients reported willingness to incur debt or use savings to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress.¹³

Minoxidil solution does not require physician office visits and is available over-the-counter.¹⁷ Despite identical ingredients, minoxidil is priced more per volume when marketed to women compared with men, which reflects the larger issue of gender-based pricing that does not exist for other AAD-approved alopecia therapies but may exist for cosmetic treatments and nonapproved therapies (eg, vitamins/supplements) that are popular in the treatment of AA.¹⁹ Oral minoxidil was more cost-effective than the topical form, and gender-based pricing was a nonissue.²⁰ However, oral minoxidil requires a prescription, mandating patients incur the cost of an office visit. Patients should be wary of gender- or marketing-related surcharges for minoxidil solutions, and oral minoxidil may be a cost-effective choice.

Diphencyprone is a relatively affordable drug for AA, but the regular office visits traditionally required for its administration increase associated cost.²¹ Self-administration of DPC at home was more cost- and time-effective than in-office DPC administration and did not decrease efficacy. A regimen combining office visits for initial DPC titration, at-home DPC administration, and periodic office follow-up could minimize costs while preserving outcomes and safety.²²

Janus kinase inhibitors are cutting-edge and expensive therapies for AA. The annual cost of these medications poses a tremendous burden on the payer (list price of annual supply ritlecitinib is $49,000),³¹ be that the patient or the insurance company. Low-dose tofacitinib may be similarly efficacious and could substantially reduce treatment costs.²³ The true utility of these medications, specifically considering their steep costs, remains to be determined.

Conclusion

Alopecia areata poses a substantial and recurring cost burden on patients that is multifactorial including treatment, office visits, concealment, alternative therapies, psychosocial costs, and missed time at work. Although several treatment options exist, none of them are definitive. Oral minoxidil and at-home DPC administration can be cost-effective, though the cumulative cost is still high. The cost utility of JAK inhibitors remains unclear. When JAK inhibitors are prescribed, low-dose therapy may be used as maintenance to curb treatment costs. Concealment and therapy costs pose an additional, largely out-of-pocket financial burden. Despite the limited efficacy of many AA therapies, patients incur substantial expenses to manage their AA. This willingness to pay reflects AA’s impact on quality of life and puts these patients at high risk for financial distress. There are no head-to-head studies comparing the cost-effectiveness of the different AA therapies; thus, it is unclear if one treatment is most efficacious. This topic remains an avenue for future investigation. Much of the cost burden of AA treatment falls directly on patients. Increasing coverage of AA-associated expenses, such as minoxidil therapy or wigs, could decrease the cost burden on patients. Providers also can inform patients about cost-saving tactics, such as purchasing minoxidil based on concentration and vehicle rather than marketing directed at men vs women. Finally, some patients may have insurance plans that at least partially cover the costs of wigs but may not be aware of this benefit. Querying a patient’s insurance provider can further minimize costs.