The galaxy presents a generally elliptical morphology, appearing largely smooth and without prominent spiral arm structures. The light profile exhibits a concentration towards the center, with a bright, yellowish core that gradually fades into a less luminous outer halo. There is a hint of slight elongation, suggesting a shape that deviates from a perfect sphere. The overall color is redder and yellowish, possibly indicative of an older stellar population and a lower rate of star formation. Some minor asymmetry or subtle disturbances can be observed in the outer regions, which could suggest past interaction or merger activity, though the galaxy appears relatively undisturbed.