The object presents as a spiral galaxy with a prominent disk. The galaxy appears relatively face-on, though with a slight tilt relative to the observer's line of sight. The spiral arms are well-defined. The central bulge has a moderate size, and exhibits a brighter, more concentrated light profile than the surrounding disk. It has a bar feature across the bulge. The spiral arms show signs of star formation, indicated by blue regions. The spiral arms are rather tightly wound. There is no visible evidence of any major merging activity, although some minor disturbances are present within the disk. The apparent color of the galaxy indicates it has undergone some star formation.
