The object presents as a system of interacting galaxies. The primary galaxy exhibits a disk-like morphology, though it appears disturbed. There is evidence of tidal features, possibly plumes or tails, emanating from the main galactic body. The light distribution is not uniform, with a bright central region and fainter, extended arms or features. The color gradients suggest the presence of differing stellar populations and dust lanes.

A secondary object, likely a smaller galaxy, is positioned nearby and appears connected to the primary galaxy via a faint bridge of material. This companion object is less resolved, but shows a brighter, more compact region suggestive of active star formation. The overall system exhibits a non-symmetrical structure indicative of ongoing gravitational interactions. There is no sign of spiral arms.
