The galaxy presents a generally smooth, elliptical morphology. There is a distinct central bulge that appears bright and concentrated. The light from the bulge appears yellowish-orange, which may indicate an older stellar population with fewer hot, young stars. The galaxy has a slight elongation and is of intermediate roundness. No significant disturbances or tidal features are apparent, suggesting it is not currently undergoing a major merger event, however there may be minor disturbances. Its size is small, appearing compact. There are no spiral arms or prominent dust lanes visible. The overall color suggests low level of star formation.
