The object presents as a singular, relatively small galaxy exhibiting a dual-lobed morphology. The primary lobe appears more elongated and diffuse, while the secondary lobe presents as more compact and of a slightly higher luminosity. There is a possible bridge of less intense emission connecting the two lobes. Overall, the light appears to be smooth with no distinct features such as spiral arms. There does not seem to be any evidence of active galactic nuclei features or significant tidal disturbances. The object is somewhat oblong, but appears closer to round than cigar-shaped.
