The galaxy presents a generally smooth and centrally concentrated light profile. Its color appears slightly redder, indicating a potentially older stellar population and/or the presence of dust. The elliptical shape, while not perfectly spherical, is significantly elongated. There is a suggestion of minor asymmetry or a faint tidal feature, although a definitive classification as an ongoing merger is uncertain from the image alone. The overall structure indicates a relatively evolved system that is likely quiescent in its star formation activity.
