The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, tending towards round, with only a subtle elongation. The central region appears brighter and more yellow/gold in color, suggesting a concentration of older stellar populations. The outer regions fade gradually, displaying a slightly bluer hue, potentially indicative of younger stars or some ongoing star formation, although it does not present a classical spiral arm structure. There is no immediately obvious indication of strong tidal interactions or major merger events; the galaxy seems relatively undisturbed. There may be some minor asymmetrical features visible, but the overall impression is of a quiescent system.
