The galaxy presents as a largely featureless, elliptical morphology, with a smooth light distribution. The color index suggests a population dominated by older stars, appearing redder than typical spiral galaxies. It exhibits a high degree of central concentration, with the light intensity diminishing gradually towards the outer regions, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy appears well-defined and unperturbed, showing no obvious signs of tidal interactions or recent mergers, although there may be minor disturbances given its classification. Its overall roundness indicates that it is most likely an E0-E3 elliptical, viewed close to face-on. The estimated size indicates a substantial physical extent. The light is most intense at the core, suggesting a possible supermassive black hole, although there is no evidence of an active galactic nucleus.
