The galaxy presents as a somewhat flattened spheroid, appearing largely smooth with subtle internal structure. There is a central, bright region that gradually fades into a diffuse halo. The light distribution indicates a dominant population of older stars, but there's a hint of bluer colors suggesting ongoing, though likely modest, star formation. The overall morphology leans toward an elliptical or lenticular type, with a slight elongation along one axis. There are no obvious signs of major mergers or significant tidal disturbances, although some minor asymmetry is visible in the outer regions of the halo.
