The galaxy presents as a moderately luminous, redshifted object. Morphologically, it exhibits characteristics of a galaxy with a dominant smooth component, though some subtle features suggest a possible disk-like structure. The overall shape is somewhat elongated, but tending towards roundness rather than a highly elliptical form. There are no obvious signs of major mergers or significant tidal disturbances, though a minor interaction is possible. The galaxy displays a color gradient, appearing bluer in the center and redder towards the edges, suggestive of a radial variation in stellar populations or dust content. The galaxy is estimated to have a substantial stellar mass, placing it among the more massive galaxies at its redshift. Its star formation rate is moderate, resulting in a specific star formation rate typical for galaxies of this type.
