The galaxy appears as a centrally concentrated, elliptical-like structure. The light profile suggests a smooth distribution, with a dominant bulge. There is an apparent lack of spiral arm structures. The galaxy's shape is somewhat elongated, but not drastically so, presenting a moderate ellipticity. The color suggests an older stellar population, likely with low star formation activity. The redshift indicates that it is a significantly distant object. The overall morphology implies a high probability of being a relatively undisturbed galaxy. The mass estimate suggests it is a massive galaxy.
