The galaxy appears to be a relatively smooth, elliptical-like structure. The central bulge exhibits a high degree of concentration, appearing bright and somewhat rounded. The light distribution fades gradually from the core outward. There is a subtle elongation to the overall shape, deviating slightly from perfectly circular. Faint indications of a possible disturbance are present, though the dominant morphology suggests a system that has largely settled into a regular form. Evidence of spiral arm structure is absent. Color gradients are subtle, but suggest a bluer central region surrounded by an area with slightly redder light. 
