The galaxy presents as a largely featureless, elliptical morphology. The central region exhibits a higher surface brightness, characteristic of a galactic nucleus or bulge. The light distribution appears smooth and centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is minimal indication of spiral arm structure or prominent dust lanes within the visible spectrum. The overall color suggests an older stellar population, although some subtle blue hues hint at ongoing, albeit modest, star formation activity. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or significant tidal interactions. The shape is nearly circular in projection.
