The galaxy appears to be a relatively smooth, elliptical-like system. Its morphology is dominated by a spheroidal component. The galaxy exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting a population of older stars. The light gradually fades from the center to the outer regions. There appears to be only a very slight disk if any, giving it a generally round shape. There is no apparent major disturbance, spiral arm structure, or signs of on-going significant merger events. There appears to be a low rate of star formation occurring within the object.