The galaxy exhibits a clear spiral structure with two prominent arms emanating from the central bulge. The arms appear somewhat tightly wound, displaying an intermediate morphology between flocculent and grand design. The bulge appears moderate in size relative to the disk, appearing mostly smooth and concentrated. The disk demonstrates a clumpy appearance, with regions of increased luminosity indicative of active star formation regions. Overall, the galaxy presents a relatively unperturbed structure, showing no major signs of ongoing merger activity, though a minor disturbance in morphology can't be ruled out. The galaxy is observed face-on and presents a notable central bar.
