The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated, bright core that gradually fades into a diffuse halo. There is a noticeable lack of distinct spiral arms or features, suggesting a generally older stellar population. The overall shape is quite round, with little to no elongation. It appears undisturbed, with no signs of ongoing mergers or major tidal interactions. Color gradients suggest that the central regions are comprised of older stars, which emits light on the redder end of the spectrum. The outer halo contains younger stars, which emit light on the bluer end of the spectrum. 