The galaxy appears to be roughly elliptical in shape, with an estimated angular size of approximately 4 arcseconds. The central region exhibits high surface brightness, appearing nearly unresolved and quite bright. A fainter, more diffuse halo surrounds the central region, extending further along the major axis of the galaxy. Faint tidal features might be present in the surrounding halo. The color of the central bulge appears consistent with an older stellar population. Overall, the morphology suggests a galaxy that has potentially undergone a minor merger in its past.
