The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, transitioning gradually to a fainter halo. The dominant color is a reddish-yellow hue in the core, suggestive of an older stellar population, while the outer regions show a slightly bluer tint, possibly indicating the presence of younger stars or some ongoing star formation. There are no discernible spiral arms or strong dust lanes visible. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers. Its shape is somewhere between round and elliptical.
