This galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape. It exhibits a bright, concentrated central bulge that gradually fades into a diffuse halo. The overall color is a bluish-white hue, suggesting the presence of some younger stellar populations, although it is also consistent with older stars. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major mergers, though a minor interaction cannot be ruled out. The light distribution suggests a relatively evolved system, potentially with ongoing, low-level star formation.
