The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. The light is generally concentrated towards the center. There appears to be some slight flattening, or ellipticity, to the overall shape, deviating slightly from a perfect circle.  Color gradients across the galaxy are subtle but potentially present; a slight color difference may exist between the very center and the outer regions. There appears to be a distinct lack of defined spiral arms or any significant dust lanes.  Overall, the galaxy seems to be undisturbed, without major signs of tidal interactions or recent mergers. Its redshift suggests it is relatively distant, and the relatively smooth light distribution is potentially consistent with a system dominated by older stellar populations.
