The galaxy presents as a relatively smooth, elliptical-like structure. The light profile suggests a concentration towards the center, with a gradual decrease in luminosity outwards. The overall color appears to be yellowish-red, indicating an older stellar population. There is no readily apparent evidence of a prominent disk or spiral arms. The morphology suggests the galaxy is fairly relaxed, with no major signs of ongoing merger activity or significant tidal disturbances, aside from the slight possible disturbances.
