This galaxy exhibits a clear spiral structure. The arms are prominent and loosely wound, with the majority of the arms appearing to be two in number. There is a distinct lack of a large central bulge. The spiral arms display knotty structures indicating active star formation. There's a hint of possible disturbances and asymmetry in the morphology, indicating potential tidal interactions. There may be ongoing merging. There is a possible weak bar feature bisecting the central region.
