The galaxy appears as a relatively smooth, elliptical or lenticular object. It is characterized by a concentrated central bulge that gradually fades into a more diffuse outer region. There is very little discernible structure such as spiral arms or dust lanes present in the image. The galaxy exhibits a color gradient, with a yellowish-white hue concentrated in the core, gradually shifting to a bluer tint in the outskirts. This suggests a population of older stars dominating the central region, with a younger population possibly contributing to the bluer color in the outer areas. The overall shape is moderately elongated, indicating that it is not perfectly spherical but slightly flattened. There is no evidence of ongoing major mergers or significant tidal disturbances. The general appearance points towards a mature galaxy with a stable configuration.
