The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Color gradients suggest a redder core region, possibly indicative of an older stellar population. The outer regions exhibit a bluer tint, implying the presence of some younger stars. There is little to no evidence of spiral arms or significant dust lanes. The overall morphology appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The galaxy displays a moderate degree of ellipticity; it is more of a disk than a perfect sphere.
