The galaxy presents as a spiral morphology, characterized by a distinct, though somewhat amorphous, central bulge. Spiral arms are clearly visible, exhibiting a grand design structure. The arms appear loosely wound, extending significantly from the central region. There are at least two prominent arms identifiable. These arms show evidence of active star formation, indicated by brighter knots and a bluer color. Some evidence of galactic disturbance suggesting an ongoing or recent merger event. This is observable through the unusual shape of the arm extending from the side of the galaxy. The disk is observed at a considerable angle. The galaxy appears to have a low bulge-to-disk ratio.
