The galaxy presents a generally smooth appearance with a dominant central bulge. There is a slight hint of a disk-like structure surrounding the bulge, though the features are not sharply defined. The color gradient suggests an older stellar population, concentrated towards the center, transitioning to a slightly bluer hue in the outer regions. The overall morphology appears relatively undisturbed, with no significant signs of major ongoing mergers, though a minor disturbance or interaction cannot be entirely ruled out. The galaxy's shape leans towards being somewhat rounded, but not perfectly spherical. The central core is very bright.
