The galaxy presents as a spiral galaxy with a moderate to small bulge size. It appears as a relatively close galaxy. The spiral arms are tightly wound and have a flocculent, or patchy structure. It seems to be mostly comprised of two spiral arms. The presence of a bar is strongly suspected to be present. There are no signs of any major or minor merging. There may be a slight smooth component in the outer areas of the galaxy. The disk is not edge on.
