The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a noticeable falloff in surface brightness towards its outer regions. The color appears to be a yellowish-orange hue, suggesting an older stellar population. There's minimal evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no major signs of ongoing mergers or tidal interactions. Its overall morphology suggests a system that is relatively evolved and potentially quiescent in terms of current star formation activity.
