The galaxy appears to be a relatively smooth elliptical galaxy, exhibiting a somewhat round morphology. A diffuse halo of light surrounds the galaxy, with a gradual decrease in surface brightness from the core outwards. The color profile suggests an older stellar population. There is little evidence of spiral arms, dust lanes, or active star formation. It does not show signs of any major merger events or strong tidal interactions. Some evidence suggests this galaxy has undergone or is undergoing minor disturbances.
