The galaxy presents as a primarily smooth, elliptical-like structure with a bright, concentrated central bulge. The core exhibits a yellowish-white hue, indicative of an older stellar population. Moving outwards from the center, the luminosity decreases, transitioning into a more diffuse halo. A subtle disc-like component might exist, but the dominant feature is the spheroidal morphology. There appears to be a possible minor disturbance or interaction with another small object at the periphery of the galaxy. Overall, the galaxy appears to be relatively isolated with no signs of major recent merger activity.