The galaxy presents as a spiral galaxy with a moderately sized bulge. A bar structure seems to be present, though possibly weak. The disk is oriented at a moderate inclination, neither face-on nor edge-on. Distinct spiral arms are visible; the winding is primarily of a medium pitch. Two main spiral arms emanate from the ends of the central bar. The color gradient suggests active star formation. There are no obvious signs of major mergers; however there appear to be some disturbances in the disk. The primary stellar population in the bulge appears old, indicated by its yellow color, while the arms suggest a younger population.
