This galaxy appears to be a spiral galaxy with a relatively small bulge. The spiral arms are well-defined and tightly wound, extending outwards from a central, elongated bar structure. The arms exhibit a granulated texture, suggesting areas of active star formation. The disk of the galaxy is oriented somewhere near face-on, with only a small amount of the dust lane visible in the spiral arms. There is no evidence of a major merger event, although there may be some minor asymmetry in the outer regions of the disk. 
