The galaxy presents as a spiral with a prominent disk structure. The spiral arms are distinct and loosely wound. A bar structure appears present traversing the central bulge. The bulge appears moderate in size relative to the disk. The galaxy is relatively smooth in appearance. The color of the bulge appears to be yellowish-orange, suggesting an older stellar population. The spiral arms exhibit a bluer hue, indicating the presence of younger, hotter stars. There is no visual evidence of major mergers or significant tidal disturbances. The disk is not edge-on. The galaxy is dominated by two spiral arms.
