The galaxy presents a generally smooth appearance with a slightly elongated, elliptical morphology. The galaxy appears to be concentrated, displaying a bright central region or core with a notable decrease in luminosity moving outwards. Its color index suggests a population of older stars, with a possible small amount of on-going star formation activity. There are no obvious signs of a major ongoing merger, though there may be slight minor disturbances or tidal features in the outer regions. Based on its morphology, it is likely an elliptical galaxy.
