This galaxy presents a relatively smooth and elliptical morphology. It appears to be somewhat elongated, with its light profile gradually decreasing from a bright central region outwards. The core appears blueish-white, suggesting the presence of a population of hot, young stars concentrated in the center. The overall color is relatively uniform, hinting at an older stellar population. There are no readily apparent spiral arms or significant dust lanes. Based on its morphology, it's likely that this galaxy is not currently undergoing any major merging events, though there is possibly some indication of minor disturbances in the outer halo.