The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge with a radial color gradient, shifting from a warmer, redder hue at the core to a cooler, greener tint towards the outer regions. The overall round morphology dominates, with a slight deviation suggesting a flattened, possibly disk-like component or the initiation of tidal interaction. The presence of the red core might indicate an aged stellar population with ongoing, albeit low, star formation. This morphology points to it being an early-type galaxy.
