The galaxy appears to be a relatively smooth, disk-shaped object with a distinct central bulge. The color profile suggests a population of older stars dominating the bulge, indicated by the yellowish hue, while the outer disk exhibits a bluer tint, suggesting ongoing star formation. While the overall structure is fairly regular, there is a slight asymmetry noticeable in the distribution of light within the disk, possibly indicative of a minor gravitational interaction or internal disturbance. There is no clear evidence of a major ongoing merger, however, it is possible that a merger may have happened in the recent past. The galaxy is moderately bright, suggesting it is a fairly massive system.