The galaxy appears to be a relatively smooth elliptical galaxy. It exhibits a concentrated central bulge that graduates outwards into a more diffuse halo. The light distribution indicates an older stellar population, lacking prominent blue star-forming regions. While a disk-like structure is not visible, the galaxy displays a slight elongation deviating from perfect circularity. No prominent tidal features or signs of major mergers are discernible in this image; though a minor disturbance cannot be ruled out. The galaxy is relatively massive, with low current star forming rate.
