The galaxy presents a generally smooth, elliptical morphology. It has a concentrated central bulge that appears yellowish, suggesting a population of older stars. The outer regions of the galaxy fade smoothly into the background, with little apparent structure such as spiral arms or prominent dust lanes. The overall shape of the galaxy is roughly circular. There is no indication of any current major merger activity, although a very slight asymmetry or minor disturbance may be present at the edges of the galaxy.
