The galaxy presents as a somewhat elongated, lenticular-like structure. The central region exhibits a bright, concentrated core, suggesting a significant stellar density and potentially the presence of a supermassive black hole. There are no distinct spiral arm features visible. The overall color appears relatively uniform, tending towards a slightly bluer hue in the center. The galaxy shows a smooth transition from the core outward, with a gradual decrease in luminosity. There are no indications of significant dust lanes or prominent star-forming regions. The galaxy's shape is mildly elliptical, and there are no indications of ongoing major mergers or tidal disturbances. The outer regions are diffuse and less defined, gradually fading into the background sky. The color profile is relatively consistent across the galaxy.