The galaxy appears to be a relatively smooth, elliptical galaxy. It has a concentrated central bulge that is more luminous than the surrounding halo. The core exhibits a slightly reddish hue, which could indicate an older stellar population in that region. The outer regions of the galaxy display a more greenish color, possibly indicating the presence of some younger stars or a different chemical composition. The overall morphology suggests that this galaxy has likely undergone little or no recent major mergers. There is no apparent disk structure or spiral arms visible. The galaxy's shape is approximately round.
