The galaxy appears as an elliptical or lenticular type system. It exhibits a smooth, concentrated light profile with a bright, yellowish core. A slight elongation is observed, with the isophotes appearing more "in-between" than perfectly round. No distinct spiral arms or prominent dust lanes are discernible. There is no obvious sign of a major merger, though there is a slight possible indication of a minor disturbance. The overall color is a moderate yellow, suggesting a stellar population that is moderately evolved. It is estimated to be a galaxy of intermediate mass.
