The galaxy appears as a moderately bright, centrally concentrated object. It exhibits a predominantly smooth morphology with a high degree of central luminosity. There is faint evidence of a possible disk structure surrounding the central bulge, indicated by a slight elongation in its overall shape, however this could also be an artifact of the imaging process. There may also be some faint tidal disturbances around the central region, possibly indicative of a minor ongoing merger, although the low level of clear disturbance means that any merger would have happened quite a while ago, or is only minor now. The core of the galaxy has a distinct blue coloration. A diffuse halo surrounds the main body of the galaxy.
