The galaxy presents as a spiral galaxy with a notable disk structure. Evidence of spiral arms is present, however they are not sharply defined. A central bulge appears to be moderate in size relative to the disk. It is important to note that this galaxy appears to have a weak bar structure. The galaxy exhibits signs of a potential ongoing merger with another galaxy. It is undergoing active star formation, as indicated by its luminosity across the observed spectrum. The overall structure of the galaxy shows some irregularity, supporting the possibility of a galactic interaction or merger event.
