The galaxy presents as a spiral system with well-defined, although somewhat flocculent, spiral arms. The arms exhibit a patchy distribution of star-forming regions, indicated by the presence of blue knots. The winding of the spiral arms appears moderate to loose, and the galaxy has at least two arms. A central bulge is visible; however, it appears relatively small in comparison to the disk component, and has a fairly small central bar structure. The galaxy's disk appears to be viewed at a slight inclination. There may be signs of mild tidal interaction or minor disturbance in the outer regions of the disk, or there may be internal features of the disk. The galaxy exhibits a gradual decline in surface brightness from the center to the outer disk regions.
