The galaxy presents as a spiral structure, with a moderately sized central bulge. The spiral arms are distinct, though somewhat fragmented, and appear to be wound relatively tightly around the galactic center. There is evidence of a possible bar structure running through the center. The disk is not edge-on, but rather presented at an angle allowing us to view the spiral arms. There are areas of star formation visible within the spiral arms. There is some evidence of a possible minor disturbance or interaction with another galaxy. The overall morphology suggests a classification of a barred spiral galaxy with active star formation.
