The galaxy presents as a centrally concentrated, relatively smooth elliptical or lenticular system. It exhibits a yellowish-white core that diffuses outward into a less defined halo. The overall shape is mostly consistent with an elliptical galaxy. There is a hint of bluer light on the outer edges which may be due to younger, bluer stars. However, overall star formation is likely low. There is no obvious evidence of recent major mergers or tidal disturbances, although minor irregularities could be present. The galaxy appears to be relatively isolated.
