The galaxy presents as a concentrated, centrally brightened object, with a significant extended halo. The central region exhibits a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy display a bluer tint, which potentially indicates recent star formation. The overall shape appears to be elliptical but is slightly perturbed. There seems to be a minor disruption on one side, which is possibly a tidal feature, merger debris, or an interacting dwarf galaxy. This disruption is also blueish in color. The galaxy displays a relatively smooth, non-spiral structure, as might be expected for an elliptical galaxy with some ongoing star formation.
