The galaxy presents a moderately inclined disk structure. Spiral arms are discernible but appear tightly wound and somewhat flocculent. These arms seem to originate near a central bulge, which appears moderate in size and brightness. The light distribution suggests the presence of a weak bar feature in the central region. The galaxy exhibits a slightly disturbed morphology, potentially indicating a minor interaction or recent merger event. Overall, the galaxy displays a relatively blue color, indicative of ongoing star formation activity within its spiral arms.
