The galaxy presents a clear spiral structure, with two prominent arms emanating from a central bulge. The winding of these arms is intermediate, exhibiting neither a tightly wound nor loosely defined morphology. The bulge appears moderate in size relative to the disk. A bar-like structure is present across the central region, with an apparent weak to moderate strength. The overall color suggests ongoing star formation. The disk shows some features, but no major disturbances indicating a recent or ongoing merger event.
