The galaxy presents as a moderately luminous object exhibiting a redshift of approximately 0.208850. It displays an elliptical morphology, tending toward a disklike shape, with a primary classification leaning toward smooth features, however, disk features are present. The luminosity profile appears to be centrally concentrated, with a bright core transitioning to a fainter extended halo or disk. The color index derived from DESI magnitudes suggests a population of older stars are present, though some star formation cannot be ruled out. The overall appearance is indicative of a massive galaxy, likely in a late stage of its evolution, potentially with a suppressed star formation rate. There is no strong indication of a major merger event, but there is a chance of minor disturbances. The galaxy appears to be inclined relative to our line of sight.
