The galaxy appears to be a spiral galaxy, exhibiting prominent spiral arms. The disk is oriented at a slight angle relative to our line of sight. A central bulge is present. The spiral arms are fairly tightly wound. There are indications of the presence of two distinct spiral arms. No major disturbances indicative of a recent major merger event are apparent, though there are slight asymmetries in the disk, suggesting potential minor interactions or disturbances. A central bar is also present. The dominant color of the galaxy is somewhat reddish.
