The galaxy presents as a merging system or a galaxy with significant tidal disturbances. Two prominent, relatively smooth components are visible, appearing yellowish-orange, indicating an older stellar population. These two components may be the remnant cores of the merging galaxies. A fainter, elongated structure connects the two brighter regions, suggesting possible tidal interactions or a bridge of material resulting from the merger. Overall, the galaxy has an irregular morphology, deviating significantly from a simple elliptical or spiral structure. There is a hint of bluer regions on the edges, which could indicate some recent or ongoing star formation. The galaxy appears elongated, with the major axis significantly larger than the minor axis. This could be due to the tidal forces stretching the galaxy during the merger process.
