The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright central bulge which appears to be comprised of older stars and a lack of dust. Fainter components extend outward from the bulge, giving the galaxy an overall elongated shape that is not perfectly round. The galaxy exhibits a yellow-red hue, indicative of a population of older stars with minimal ongoing star formation. No spiral arms or significant dust lanes are readily apparent. There is possibly a small indication of a minor disturbance in the galaxy's halo.
