The galaxy presents as a flattened elliptical or possibly a lenticular galaxy, viewed at a significant inclination relative to our line of sight. The light distribution is relatively smooth and centrally concentrated, with the highest luminosity located centrally. A gradual decrease in luminosity is observed moving away from the core toward the outer edges of the galaxy. The overall color appears to be moderately red, suggesting a population of older stars. However, bluer regions are also present in the outskirts, indicating ongoing or recent star formation activity there. No distinct spiral arm structures are observed and there are no signs of tidal tails or strong disturbances, which suggests the galaxy is not currently undergoing a major merger. However, there may be minor disturbances present. The galaxy is rather faint overall, suggesting it is either a dwarf galaxy or a more massive galaxy located at a considerable distance.
