The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a fairly homogenous distribution of light outwards. The primary color of the galaxy is yellow/orange, suggesting an older stellar population and a cessation of significant star formation. The light profile suggests it has a high degree of central concentration, with a relatively quick falloff in surface brightness moving outwards from the center. There are hints of disturbances to one side of the galaxy. The overall morphology indicates a system that has likely undergone significant dynamical relaxation.
