The galaxy presents as a grand design spiral structure, though moderately inclined from our line of sight. It exhibits two prominent spiral arms emanating from the central bulge region. The arms appear relatively well-defined and symmetrical.

The central bulge is moderately sized, displaying a yellowish-white hue indicative of an older stellar population. The spiral arms show a bluer color, suggesting more recent star formation activity and the presence of younger, hotter stars. Patches of increased blue intensity are visible within the arms, likely representing star-forming regions. There is a possible bar structure through the center. The galaxy shows no signs of major merger activity.
