The galaxy presents as a moderately bright, elongated object with a noticeable central bulge. Its overall structure appears relatively smooth, though there are hints of disk-like features extending outwards from the bulge. The color distribution indicates a dominant population of older stars, particularly within the bulge, which exhibits a yellowish hue. Fainter, bluer regions may be present in the outer areas of the galaxy, suggesting some ongoing, though perhaps limited, star formation. There is a slight asymmetry in its morphology, possibly indicative of minor gravitational interaction or internal disturbances. No strong evidence of major mergers or tidal tails are immediately apparent in this image.
