The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears slightly elongated along its major axis. The color gradient suggests an older stellar population in the core, indicated by the reddish hue, transitioning outwards to a bluer halo, implying ongoing or recent star formation in the outer regions. No significant tidal features or signs of major mergers are immediately apparent, though subtle asymmetries may indicate minor interactions. The overall structure is consistent with an early-type galaxy undergoing a transitional phase, potentially evolving from a spiral to an elliptical form or experiencing late-stage star formation in its outskirts.
