The galaxy presents a relatively smooth, elliptical morphology. Its core exhibits high luminosity, suggesting a high density of stars or potentially an active galactic nucleus, though the image alone cannot confirm this. The galaxy's color profile appears generally redder, possibly indicating an older stellar population with lower rates of current star formation. There is little evidence of spiral arm structure or prominent dust lanes. The isophotes, or lines of equal brightness, appear largely round. There is no obvious visual indication of a major ongoing merger event, although some minor asymmetry might be present in the outer regions. Overall, this galaxy seems consistent with a classification of a massive elliptical galaxy with a substantial stellar mass and a quiescent star-forming environment.
