The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated bulge with a somewhat diffuse halo or envelope surrounding it. The core region displays a yellowish hue, likely indicating an older stellar population and relatively low levels of ongoing star formation. The overall shape appears mostly round, with a slight elongation. There are no distinct spiral arm structures visible, nor is there evidence of strong tidal disturbances or a major ongoing merger. Faint extensions or diffuse structures appear to extend away from the main body of the galaxy. The central part of the galaxy is substantially brighter than the halo.
