The object appears to be an interacting galaxy system. The primary component presents as a luminous disk galaxy. The overall color of the primary galaxy is suggestive of an older stellar population. A secondary galaxy, possibly a dwarf galaxy, is observed close to the primary. There are indications of tidal distortions and possible merging activity within this system, potentially a major merger. The system shows some irregular structures, suggestive of ongoing gravitational interactions. The overall form of the object could be described as disturbed.
