The galaxy presents as a merging system or a galaxy undergoing a significant interaction. The morphology is highly disturbed, characterized by an irregular shape with two distinct, bright nuclei suggestive of either a galaxy merger or a galaxy with a highly active galactic nucleus in each lobe. Faint tidal features or extended stellar halos are possibly present, though blending with background sky and other galaxies cannot be ruled out. There is no strong evidence of a prominent disk component. The overall color index suggests a population that is not strongly dominated by either old red stars or young blue stars. This could indicate an intermediate stellar population or a mix of both. A presence of active star formation is possible, especially in the vicinity of the nuclei. The spiral arms are loosely defined and disturbed. The presence of a bar cannot be ruled out. The Bulge is moderate in size.
