The galaxy appears as a centrally concentrated elliptical structure with a smooth, diffuse morphology. Its core is a bright, yellowish-white, indicating a possible presence of an older stellar population. The galaxy transitions outwards to a less luminous, reddish halo, potentially indicative of a lower density of stars and/or a higher proportion of older, redder stars. There are no visible signs of spiral arms or a prominent disk. There is no indication of major disturbances or merging activity.
