The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. Its color appears slightly greenish, potentially indicating some level of ongoing star formation within the galaxy, although the overall smoothness suggests a dominant older stellar population. There is no discernible structure such as spiral arms or a prominent disk. Slight asymmetry may be present, but no evidence of major mergers or tidal disturbances are visible within this image. The galaxy seems to exist as a fairly isolated system, showing no obvious close companions.
