The galaxy appears to be a somewhat flattened elliptical or lenticular type, displaying a smooth, centrally concentrated luminosity profile. It is generally diffuse, with a noticeable bulge dominating the central region. The galaxy exhibits a faint, extended halo surrounding the core, its edges fading gradually into the background. The overall color appears relatively red, indicating an older stellar population. A faint ring or shell-like structure is observed to the lower left, possibly indicative of a past merger event. No distinct spiral arm structures are visible. Overall, this galaxy gives the impression of a fairly evolved system with ongoing or recently ceased star formation.
