The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile with a gradual decrease in surface brightness towards its outer regions. The core shows a notable reddish hue, potentially indicative of an older stellar population or significant dust obscuration. The overall shape appears largely spheroidal, deviating only slightly from perfect circularity. There is no visually apparent evidence of spiral arm structure, bar features, or significant tidal disturbances, with minimal asymmetry. A very faint, diffuse halo surrounds the main body of the galaxy, extending to a limited degree. Overall, the galaxy appears well-defined and relatively undisturbed.
