The galaxy presents as a spiral galaxy, observed at an oblique angle. The central bulge appears moderately sized, exhibiting a bright concentration of light. The spiral arms are well-defined and extend outwards from the central bulge, displaying a relatively loose winding pattern. Two dominant arms appear especially prominent. There is some indication of a bar-like structure traversing the central region of the galaxy. The galactic disk shows regions of increased activity, evidenced by patchy areas of differing color, suggestive of on-going star formation. There appear to be some disturbances throughout the main body of the galaxy.
