The galaxy presents as a relatively smooth, elliptical-like object, with no apparent spiral arm structures. The core region appears quite bright and concentrated, exhibiting a yellowish-orange hue, suggesting a population of older stars and a lack of significant ongoing star formation. The outer regions fade gradually, showing a more reddish color profile, again indicative of an aging stellar population. There is no prominent dust lane or other features indicating active galactic nuclei activity within the resolution of the image. The overall appearance suggests a galaxy that is relatively evolved, possibly an early-type galaxy that has largely exhausted its gas reserves for star formation. There are no obvious signs of tidal disturbances or ongoing mergers, indicating a likely quiescent state.
