The galaxy presents as a relatively smooth, elliptical form. There is a concentrated central bulge, and an extended halo or envelope of stars. Coloration suggests an older stellar population dominating the light output, particularly in the core. The outer regions appear somewhat bluer, potentially indicating some ongoing, albeit limited, star formation in that area. No distinct spiral arm structures are visible, nor are there any obvious signs of a major ongoing merger event. There might be a minor disturbance, or some minor distortions in the symmetry of the outer regions. Overall, the galaxy appears to be a fairly evolved system with a dominant spheroidal component.
