The galaxy presents as a generally smooth and centrally concentrated object. There is no apparent spiral structure or significant dust lane obscuration. The light distribution suggests an elliptical morphology, with a high degree of circularity. The core exhibits a bright, unresolved nucleus indicative of high stellar density. The galaxy appears to be relatively isolated, with no obvious tidal features or nearby interacting companions. There is a slight color gradient, with a bluer hue towards the outer regions, possibly indicating a difference in stellar populations or recent star formation activity away from the galactic center.
