The galaxy presents as a single, well-defined object with a generally smooth, round appearance. The light is centrally concentrated, displaying a gradual decrease in intensity toward the outer regions. There is a subtle color gradient, with a slightly yellower hue at the core transitioning to a somewhat bluer tone in the outer areas. No distinct spiral arms or prominent dust lanes are discernible. There is no strong evidence of any ongoing major mergers or tidal disruptions affecting the galaxy's structure. Minor irregularities in the light distribution might suggest the presence of subtle internal features or past interactions. The overall morphology is consistent with that of an elliptical galaxy or a lenticular galaxy seen at a significant distance.
