The galaxy presents as a fairly smooth, centrally concentrated object, likely an elliptical galaxy or a lenticular galaxy viewed face-on. The light distribution suggests a spheroidal morphology, with a high degree of radial symmetry. The color gradient indicates a general trend from a yellower core region to slightly bluer outer regions. This color difference may be due to the presence of younger stellar populations and a small amount of on-going star formation in the outer regions, as opposed to the older stellar populations that are dominant toward the center. There is no visual evidence of spiral arms or a prominent disk. There are no significant signs of tidal disturbances or mergers, but that does not mean that one has not happened in the past. Overall, the galaxy appears to be relatively undisturbed morphologically.
