The galaxy presents as a somewhat elliptical structure, exhibiting a centrally concentrated luminosity profile indicative of a substantial bulge component. The dominant color in the core is yellowish-white, suggesting an older stellar population. A slight extension is observed on one side, appearing as a fainter, elongated region with a bluer tint. This could represent a tidal feature resulting from a minor gravitational interaction or potentially a distorted disk component. The overall smoothness of the galaxy suggests it is relatively undisturbed, though subtle irregularities might indicate ongoing or past interactions. The galaxy appears relatively compact, with a modest apparent size. 
