The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge that exhibits a yellow-orange hue, suggesting a population of older stars. Fainter, diffuse light extends outwards from the core, fading into the background. There appears to be little discernible structure, such as spiral arms or dust lanes. It appears to be somewhat round, though slightly elongated. There is no visible evidence of tidal tails or other signs of major interactions or recent mergers.
