This galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology, with a brighter, yellowish core that gradually fades into a less luminous, more diffuse halo. There is evidence of some bluer star formation regions in the outer parts of the galaxy, which could indicate ongoing or recent star formation. These regions appear somewhat patchy and irregular in distribution. There is no immediately obvious evidence of strong tidal features or major disturbances, suggesting that the galaxy is relatively undisturbed. The galaxy appears slightly round in shape, without a cigar-shaped appearance. It seems unlikely that the galaxy is undergoing a major merging event.
