The galaxy presents a generally smooth and rounded morphology. The light profile suggests a concentration of older stellar populations toward the galactic center. The redder hue of the central region supports this, indicating a likely bulge component dominated by evolved stars. The outer regions exhibit a bluer coloration, which suggests the presence of some younger stellar populations, but overall the galaxy appears to have a limited amount of ongoing star formation. There are no obvious signs of spiral arms or a disk-like structure. No major disturbances in the overall structure are seen, indicating that the galaxy has likely not undergone a major merger event recently. Overall, this galaxy appears to be a relatively undisturbed, massive elliptical galaxy with limited current star formation.
