The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a concentrated, bright core with a yellowish-orange hue, suggesting an older stellar population. Moving outwards from the center, a gradual decrease in luminosity is observed. The outer regions display subtle hints of a disk-like structure with a faint bluish tint, possibly indicating the presence of some younger, hotter stars or ongoing star formation. There are only minor disturbances visible in the structure of this galaxy. The galaxy appears to be relatively round in shape. Overall, the galaxy appears to be a large, massive system with a mixture of stellar populations and only some current star formation.
