The galaxy appears to be a relatively smooth, elliptical system. Its core exhibits a reddish hue, possibly indicating an older stellar population dominating the central regions. The outer regions are less well-defined and display a bluer tint, which could be evidence of ongoing or recent star formation, albeit at a low rate. The overall morphology suggests a lack of significant spiral arms or a prominent disk structure. There are no obvious signs of a major ongoing merger, but the presence of minor disturbances cannot be completely ruled out from this image alone. The galaxy's shape is largely round, with minimal elongation.
