This galaxy presents a smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, compact core. The light distribution decreases gradually outwards, showing a nearly round shape with a slight elongation. The overall color suggests a dominant population of older stars, with a subtle bluer halo hinting at some ongoing or recent star formation activity, albeit at a low level. There appears to be no prominent spiral arm structure or dust lanes visible within the galaxy. No signs of any major mergers or disturbances are visible.
