The galaxy presents as a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, suggestive of a significant stellar population or potentially an active galactic nucleus. The light gradually decreases in intensity moving outward from the core. There is a subtle disk like structure, with areas of less light concentration. The overall color profile indicates a population of older stars, though there might be a small amount of star formation. There is also a possible interaction with a nearby object, but this could also be a star behind it.