The galaxy presents as a relatively compact, elliptical system. The light distribution is dominated by a smooth, centrally concentrated bulge. There is little evidence of spiral arm structure or significant dust lanes. The overall color suggests an older stellar population, potentially comprised largely of evolved stars. Given its relatively homogenous appearance, this galaxy likely has a low star formation rate. It exhibits a moderate inclination, and is neither perfectly spherical nor highly elongated. There is no immediate visual evidence of a major ongoing merger event or significant tidal disturbances, though minor disturbances can not be ruled out. 
