The galaxy presents as a yellowish-white, moderately elliptical object. Its light is relatively smooth and centrally concentrated, indicating a possible lack of significant star formation activity. The galaxy appears to be relatively isolated with no clear signs of major interaction with other galaxies or gas clouds, although a minor disturbance cannot be fully excluded. The galaxy does not present a clear disk or spiral arm structure. Its overall shape suggests a galaxy transitioning toward, or already being a more spheroid-dominated system. The colour indicates a prominence of older stellar populations.
