The galaxy presents an elliptical morphology, with a smooth, diffuse light profile. The central region is dominated by a yellowish-white hue that graduates to a warmer color, potentially indicating a population of older stars concentrated towards the core. There is a lack of distinct spiral arm structures or prominent dust lanes visible. The outer regions of the galaxy fade gently into the background sky, suggesting a gradual decrease in stellar density. The overall structure appears largely undisturbed, with no obvious signs of tidal interactions or major mergers.
