Identification of a novel mutation in the KITLG gene in a Chinese family with familial progressive hyper- and hypopigmentation

Abstract

Background: Familial progressive hyper- and hypopigmentation (FPHH, MIM 145250) is a rare hereditary skin disorder that is predominantly characterized by progressive, diffuse, partly blotchy hyperpigmented lesions intermingled with scattered hypopigmented spots, lentigines and sometimes Cafe-au-lait spots (CALs). Heterozygous mutations of the KIT ligand (KITLG, MIM 184745) gene are responsible for FPHH. To date, only eight KITLG mutations have been reported to be associated with FPHH, and no clear genotype-phenotype correlations have been established. This study aimed to identify the causative mutations in the KITLG gene in two Chinese FPHH patients.Methods: Direct sequencing of the coding regions of KITLG was performed. Pathogenicity prediction was performed using bioinformatics tools, including SIFT, Polyphen2, and SWISS-MODEL, and the results were further evaluated according to the 2015 American College of Medical Genetics and Genomics (ACMG) guidelines.Results: The novel mutation c.104A>T (p.Asn35Ile) and the recurrent mutation c.101C>T (p.Thr34Ile) in KITLG were identified. As shown using SIFT and Polyphen-2 software, both mutations identified in this study were predicted to be detrimental variations. Three-dimensional protein structure modeling indicated that the mutant KITLG proteins might affect the affinity of KITLG for its receptor, c-KIT. According to the 2015 ACMG guidelines, the novel mutation c.104A>T was ‘likely pathogenic’.Conclusions: To date, most of the identified KITLG mutations have been clustered within the conserved VTNNV motif (amino acids 33-37) in exon 2. The known mutations are only involved in 33V, 34T, 36N, and 37V but not 35N. We have now identified a novel mutation in KITLG, c.104A>T, that was first reported in FPHH within the conserved 35N motif. These results strengthen our understanding of FPHH and expand the mutational spectrum of the KITLG gene.