The galaxy appears as a somewhat elliptical, centrally concentrated structure. Its light profile seems smooth with no distinct spiral arms, bars, or other features typically associated with disk galaxies. The core region appears brighter and slightly yellowish, perhaps due to a population of older stars. The galaxy exhibits a moderately compact size and a smooth distribution of stellar light across its surface, suggesting it could be an elliptical galaxy at a considerable distance. Based on its color and morphology, the galaxy appears to have a relatively high mass, a low star formation rate and a red color. A significant portion of citizen scientists observing this object classified it as smooth. There is some indication of possible minor disturbances or mergers, but the main body of the galaxy is relatively undisturbed.
