The galaxy appears to be a relatively smooth, elliptical-like structure with a high degree of central concentration. Its light profile suggests a centrally dominant bulge. There is a slight elongation, but overall, the galaxy appears nearly circular.

There is a suggestion of a subtle color gradient, where the central region appears slightly more yellow-white, transitioning to a bluer hue in the outer regions. This may be due to differing stellar populations.

There are no obvious signs of strong tidal disturbances or ongoing major mergers. Close inspection of the galaxy suggests the possibility of minor asymmetries or faint features that might suggest past minor interactions or accretion events, but the overall appearance indicates a relatively relaxed and settled system.
