The galaxy presents as a moderately luminous, early-type system at a significant redshift. Its morphology appears predominantly smooth and elliptical in shape, with a high degree of roundness. There is a possible slight flattening, but it is difficult to resolve finer structures at this distance. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The red color suggests an older stellar population. There is a slight indication of a central bulge, or at least a centrally concentrated brightness profile, but this is subtle. No distinct disk component or spiral arms are apparent in the image. Based on the data, the galaxy exhibits a low star formation rate.