The galaxy presents as a centrally concentrated object with a smooth, largely featureless appearance. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the color gradually transitions to a more diffuse, bluish-white, indicative of a younger stellar population or ongoing star formation in the outer regions, although this is subtle. The overall shape approximates a round to slightly elliptical morphology. There's no obvious indication of a spiral arm structure or significant dust lanes, which is consistent with an early-type galaxy. The galaxy appears to be relatively isolated, with no clear signs of recent or ongoing mergers or tidal disturbances, though there are some minor color differences in the outskirts. The galaxy is relatively compact, with a moderate radial extent.
