The galaxy presents as a relatively compact object with an elliptical morphology. It exhibits a smooth light distribution, with a radial color gradient shifting from redder hues in the central region to bluer colors towards the outer edges. The structure appears largely undisturbed, although there is faint evidence of a possible minor tidal interaction or disturbance in the form of slightly distorted isophotes. The central region is luminous, indicating the presence of either a dense stellar population or an active galactic nucleus. The overall appearance suggests a galaxy that has largely completed its major mergers, and is undergoing a period of relative quiescence.
