The galaxy appears as a relatively smooth, elliptical-shaped object. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards. The color gradient suggests a population of older stars, with a dominant redder hue. There is no apparent disk or spiral structure, though some faint and subtle asymmetries are present that may indicate a minor disturbance or interaction. There is no noticeable star formation activity, with the galaxy predominantly exhibiting a quiescent morphology. The overall structure appears fairly undisturbed, without significant signs of a major merger or tidal disruption. The galaxy is relatively round in appearance, lacking a strong elongated shape.
