The galaxy presents a largely smooth, elliptical morphology. There is a bright, concentrated central bulge that appears yellowish in color, indicative of an older stellar population. Surrounding the bulge, a more diffuse halo extends outwards, displaying a bluer hue, possibly suggesting some ongoing or recent star formation. However, the blue component appears relatively subdued. The galaxy exhibits a generally round shape with no obvious signs of strong tidal disturbances or major mergers, although there might be a subtle asymmetry in the outer halo suggestive of a minor interaction. Overall, the galaxy gives the impression of being a relatively quiescent system with a dominant, evolved stellar population.
