The galaxy presents a moderately inclined disk, characterized by a prominent bulge. The bulge appears luminous and concentrated, suggesting a high stellar density and potentially an older stellar population. Faint spiral arm structures are observed extending outwards from the central region, though these arms are tightly wound. There is a slight asymmetry in the galaxy's overall light distribution. A faint bar feature may be present, but its presence is not definitive due to the galaxy's moderate inclination. The galaxy's outer regions exhibit a gradual decrease in brightness, without a sharply defined edge. Overall color indices suggest moderate levels of ongoing star formation activity.
