This galaxy exhibits a prominent spiral structure. The arms appear relatively tightly wound around a central bulge. The bulge constitutes a moderate proportion of the galaxy's overall size. The spiral arms themselves display a somewhat patchy or flocculent appearance, with discernible variations in brightness and color suggesting regions of differing stellar populations and dust content. The galaxy presents a distinct disk-like morphology when viewed face-on. There is no apparent significant interaction or merging events presently occurring based on the smoothness of the disk. There may be a faint bar feature that crosses the central bulge. 
