This galaxy presents as a relatively smooth and centrally concentrated object. It exhibits a dominant elliptical morphology, appearing mostly round, with a gradual decrease in luminosity from its core. The core region is bright and exhibits a yellow-ish hue, potentially indicating an older stellar population. The galaxy displays a relatively uniform color profile across its extent, with a slight reddening at the edge of the galaxy. It does not appear to show any strong signs of spiral arm structures, tidal features, or significant ongoing mergers, though there could be a minor disturbance or interaction with another galaxy. There is some indication of dust extinction, possibly in a disk or ring surrounding the galactic core. The overall appearance suggests a galaxy that has largely completed its major mergers and star formation and is evolving passively.
