The object presents a roughly elliptical morphology, appearing somewhat compact. The central region exhibits a high surface brightness, with a color profile indicating substantial blue light emission. A fainter, diffuse halo surrounds the core, extending further along one primary axis giving the galaxy a slightly distorted appearance. There is some subtle evidence for dust lanes or patchy extinction within the halo. Faint color variations are detectable within the disk, but its overall structure appears largely amorphous. Close inspection does not show tightly wound spiral arms or a well-defined bar structure. Faint tidal features cannot be ruled out, but there is no conclusive evidence for a recent major merger event.
