The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a noticeable decrease in luminosity as you move outward. The color gradient suggests a dominant population of older stars, indicated by the yellowish-red hue within the core, transitioning to a slightly bluer halo, possibly indicating some ongoing, albeit limited, star formation. The overall structure appears undisturbed, showing no significant signs of tidal interactions or major merging events. The galaxy displays a flattened shape but is largely considered in between a disk and fully spherical galaxy. It does not appear to be actively merging. There may be a slight perturbation in the galaxy’s smoothness.
