The galaxy appears to be a relatively large elliptical, exhibiting a smooth, diffuse morphology. The light profile shows a concentration towards the center, which may indicate the presence of an actively accreting supermassive black hole. The galaxy exhibits a color gradient, with the central regions appearing yellow and the outer regions appearing more green and purple. The overall color is consistent with an older stellar population, with limited ongoing star formation. The galaxy's shape is roughly in between round and cigar-shaped, appearing somewhat oblong, but not highly elongated. There does not appear to be any evidence of merging or major disturbances in the system. The estimated size based on the half-light radius suggests that this is a relatively large galaxy.
