The galaxy presents as a spiral type, observed at an angle somewhere between face-on and inclined. A disk structure is apparent. The spiral arms are resolved, and it appears there are two dominant arms winding their way out. The winding is somewhere in between tight and loose. The central bulge is estimated to be of small size. There is a bar structure in the center of the galaxy. There does not appear to be a major merger occurring, though there may be some minor disturbances present.
