The galaxy appears to be a relatively smooth, elliptical-like system. It displays a bright, concentrated central bulge that gradually fades into a more diffuse outer halo. There is a slight elongation, tending towards an in-between rounded shape, but overall the structure lacks any significant disk-like features or spiral arm structures visible in the image. No signs of major mergers or tidal disturbances are apparent, but a minor disturbance cannot be ruled out. The galaxy's color profile suggests a stellar population that has moderate recent or ongoing star formation within the system.
