The galaxy presents as a roughly elliptical, lenticular-like object. The central region exhibits a concentrated luminosity profile with a yellow-white hue. The outer regions display a smoother, fainter distribution of light, transitioning into an orange-red color, suggesting an older stellar population in the outskirts.

There is a suggestion of a very subtle disk, however no spiral arm structure or bar is discernible. No strong dust lanes are apparent. The galaxy appears relatively undisturbed, showing no significant tidal features or morphological distortions indicative of a recent major merger. 
