The galaxy presents as a disk galaxy, viewed at a moderately inclined angle. It exhibits a prominent disk structure with spiral arms. The spiral arms are well-defined, numerous, and have a generally tightly wound morphology. There is evidence of clumpy star formation within the arms, indicated by localized brighter regions. The galaxy possesses a notable bulge component, estimated to be of moderate size, with a bar structure oriented across its center. There is a notable dust lane is obscuring the galaxy. There is no clear sign of a major merger or significant tidal disturbance.