The galaxy exhibits a generally smooth morphology, with a centrally concentrated bulge region. The overall shape is ellipsoidal, appearing somewhat elongated along one axis. The color gradient suggests an aging stellar population, trending towards redder hues. There is a subtle hint of disk-like structure extending from the central bulge, however, distinct spiral arms are not discernible. The galaxy shows no obvious signs of recent or ongoing major merger activity, though there is some minor asymmetry in the outer regions.
