The galaxy presents a largely smooth and rounded morphology. The core region exhibits high luminosity, indicating a concentrated stellar population and possibly an active galactic nucleus. The light profile appears relatively uniform, with a gradual decrease in brightness from the center outwards. There is no visual evidence of spiral arms, bar structures, or significant dust lanes. A slight color gradient is observed, with a yellowish tint towards the center, possibly indicating an older stellar population, transitioning to a bluer hue in the outer regions, which may point to younger stars. There are no obvious signs of ongoing major mergers or tidal disturbances. The overall structure suggests a probable elliptical galaxy.
