The galaxy exhibits a mostly smooth morphology, with a dominant central bulge. The light distribution indicates an elliptical shape, more leaning towards an "in between" ellipticity rather than perfectly round or highly elongated. A disk is faintly discernible, but not prominent. There is no obvious evidence of major mergers or strong tidal disturbances, although there might be a hint of minor disturbance. The central bulge is yellowish-orange, suggesting an older stellar population. There is a very low level of star formation.
