This galaxy presents as a fairly smooth, elliptical system. The central bulge exhibits a high degree of sphericity, displaying a concentrated luminosity gradient transitioning outwards to a fainter, more diffuse halo. There is no immediately apparent disk structure or spiral arm morphology within the visible light spectrum. The galaxy appears relatively undisturbed, with no evidence of major mergers or significant tidal interactions. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue of the central bulge. The outer regions exhibit a slightly bluer tint, hinting at the presence of a younger stellar population, or low levels of on-going star formation. The overall morphology is consistent with a relatively quiescent, evolved galaxy.
