The galaxy presents a generally smooth morphology with a concentrated central region. It appears elliptical, deviating slightly from a perfectly circular shape. There is a subtle color gradient, transitioning from a bluish-white core to more diffuse, slightly reddish outer regions. This suggests a population of younger, hotter stars in the central region with older, cooler stars more dispersed towards the edges. Faint hints of a disk-like structure may be present, though not clearly defined. There are no obvious signs of major mergers or significant tidal disturbances, although some minor asymmetry or faint streams cannot be ruled out. The light distribution appears to be centrally concentrated, indicative of an early-type galaxy.
