The galaxy appears to be an elliptical or lenticular type, characterized by a relatively smooth, featureless morphology. The light distribution suggests a concentrated central bulge which fades gradually outwards. The shape is approximately between round and elliptical. The overall color is yellowish-orange, indicating an older stellar population, relatively lacking in young, massive stars. There is some evidence of minor disturbances in the galaxy's structure. This might indicate past minor merger events.
