The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, centrally concentrated light distribution, with the highest intensity observed towards the core. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue. There is no apparent spiral arm structure or significant dust lane obscuration visible in the image. The galaxy appears to be relatively undisturbed, without any signs of major mergers or tidal interactions. The overall morphology suggests a system that has undergone significant dynamical relaxation, possibly with little ongoing star formation.
