The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration with a relatively small, bright core, indicating a likely evolved stellar population. The overall color appears to be yellowish-orange, suggesting older stars dominate the galaxy's stellar population, with a lower rate of ongoing star formation. While predominantly smooth, a subtle disk-like structure may be present, as there is a slight elongation, but is not as easily visible as it is with spiral galaxies. There is no obvious evidence of major mergers or tidal disturbances and the galaxy seems to exist as an isolated system.
