The galaxy appears to be a relatively smooth, elliptical-type galaxy with a high degree of central concentration. It exhibits a slightly elongated morphology. The galaxy displays a color gradient, with a brighter, redder core region transitioning to a bluer halo or outer disk. There is little to no visual evidence of spiral arm structure or significant dust lanes. Based on its morphology, it is likely a relatively massive galaxy undergoing a low rate of star formation. There is also no visual evidence of any major mergers or strong tidal disturbances.