The object presents as a relatively compact galaxy, with a central bright core, possibly an active galactic nucleus or a region of intense star formation. The light is centrally concentrated with a radial decrease in intensity. The isophotes appear nearly circular, suggesting a classification toward the elliptical or lenticular end of the Hubble sequence. There is indication of possible tidal features or minor disturbances present surrounding the galaxy. There may be asymmetry in the outer regions of the galaxy.
