The galaxy presents an elliptical morphology, appearing largely smooth with a diffuse outer region. The light distribution is centrally concentrated. There may be an indication of a recent or ongoing merger event, suggested by the presence of two distinct, albeit overlapping, luminous cores. There is a slightly disturbed appearance to the galaxy, but the disturbance is fairly minor. The overall color is somewhat reddish, indicative of an older stellar population and lower levels of current star formation within the galaxy. Based on the size, the galaxy is probably quite massive.
