The galaxy appears to be a spiral type, exhibiting a disk-like structure. The spiral arms are relatively well-defined. There is a notable central bulge. The galaxy is viewed at an angle somewhat between edge-on and face-on. Moderate star formation may be occurring within the disk, but not at a high rate. There may be a bar structure present within the galaxy, or the spiral arms could be tightly wound. The core is relatively smooth and does not show any apparent disturbances, although minor disturbances can not be ruled out. 
