The galaxy presents as a spiral galaxy, displaying a clear disk structure. Spiral arms are discernible, with a slightly flocculent morphology. There appears to be a modest central bulge, and no clear bar feature. The arms exhibit a moderately wound morphology. Indications are that it has between one and three main spiral arms. There are possible signs of minor disturbances in the galaxy's structure, suggestive of a potential gravitational interaction or recent merger event. The galaxy appears to be undergoing active star formation, as evidenced by its bluer color.