The galaxy presents as a moderately bright, elliptical-shaped structure. Its color appears to be a pale bluish-white, indicating the presence of a population of younger, hotter stars, however the relatively smooth light distribution suggests that it may be mostly composed of older stars. There are no obvious spiral arms or dust lanes. The galaxy appears somewhat compact in size. The overall impression is of a galaxy undergoing, or having undergone, a period of active star formation, and seems relatively undisturbed. Based on its morphology, this galaxy seems to be an elliptical galaxy of intermediate mass and a relatively small star formation rate.
