The galaxy presents as a primarily smooth, elliptical morphology. It exhibits a centrally concentrated bright bulge that fades into a more diffuse halo. There is a hint of disk structure, but this is not well defined. There are some disturbances and potential interactions with nearby objects, and possible signs of merging activity. The galaxy is generally round in shape, but slightly elongated. The light profile appears relatively smooth and featureless, with no prominent spiral arms or dust lanes visible in this imagery. The overall color is yellowish, suggesting a population of older stars and a lack of significant ongoing star formation.
