The galaxy presents as a relatively smooth, elliptical-like structure. The primary body exhibits a concentrated, bright central bulge that transitions smoothly into a more diffuse outer halo. A noticeable asymmetry is apparent, with an extended, faint feature on one side suggesting a potential tidal interaction or recent minor merger. The dominant color is redder, possibly indicating an older stellar population and a diminished rate of star formation. Overall, the galaxy appears relatively isolated and undisturbed, aside from the asymmetry, which is visible in the halo region of the galaxy.
