The galaxy presents a discernible spiral structure. At least three spiral arms appear to emanate from a central bulge. The arms display a somewhat tightly wound morphology, appearing to originate near the center of the galaxy. The color gradients suggest active star formation regions along the spiral arms. There is a defined central bulge, but it is not overly prominent. The galaxy shows no obvious signs of major mergers or significant tidal disturbances. A weak bar feature may be present, however it is not very obvious. There is evidence of both disk and spiral structure.