The galaxy presents as a singular, albeit somewhat disturbed, luminous structure. Its overall morphology appears largely elliptical, displaying a smooth light profile with a marked central concentration and a gradual decline in luminosity towards its outer edges. The primary color appears to be a golden hue, possibly indicating an older stellar population dominating its light output. There is a non-negligible, but not dominant, disturbance in its morphology, which may be an indication of a minor ongoing or past merger event. The observed light distribution suggests a system with little to no ongoing significant star formation, further supporting the conclusion that the galaxy is comprised of mostly older stars.
