The galaxy presents as a relatively smooth, elliptical structure. The light profile is generally concentrated toward the center. There is a slight elongation in the galaxy's shape; however, it is mostly round. The light emitted is predominantly redder in the core, with a more yellow tinge towards the outer regions of the galaxy. There appears to be no indication of significant disturbances, like tidal tails or other obvious merger remnants. The galaxy appears relatively isolated, without a dominant spiral structure.