The galaxy presents as a somewhat elongated, centrally concentrated object. It exhibits a relatively smooth light distribution, lacking prominent spiral arms or distinct morphological features typically associated with disk galaxies. The color gradient appears subtle, with a slightly redder core region transitioning to a bluer halo. There's no evidence of ongoing major merger activity or significant tidal disturbances in the immediate vicinity, although a minor asymmetry in the light distribution might suggest a past interaction or internal dynamical process. Given the overall appearance, a classification as an early-type galaxy, potentially an elliptical or lenticular, is plausible.
