The galaxy exhibits a discernible spiral structure, characterized by multiple, loosely wound arms. The arms display a patchy appearance, suggesting active star formation regions. The central bulge appears relatively small and less prominent compared to the overall disk size. The galaxy shows a slight disturbance in its morphology, possibly indicating a minor interaction or past merger event. There is no clearly visible bar structure. The disk is oriented close to face-on. The galaxy appears relatively blue, implying ongoing star formation.
