The galaxy presents as a spiral type. The central bulge appears moderate in size, with a yellow/orange hue, potentially indicative of an older stellar population. Two well-defined spiral arms extend from the bulge, demonstrating a grand design structure. The arms exhibit a tightly wound morphology.  Within the spiral arms, there is a distinct bluer color, indicating the presence of younger, hotter stars, and active star formation regions. The galaxy exhibits no signs of major mergers, though possible disturbances are not excludable.  The disk is viewed at a nearly face-on orientation. A bar structure is weakly present across the central region.
