The galaxy presents as a face-on spiral with prominent arms extending from a central bulge. The spiral arms are loosely wound, displaying a patchy distribution of star formation regions, indicated by variations in color. The central bulge appears moderate in size. The disk component shows evidence of ongoing star formation. No obvious signs of a major merger are apparent, although minor disturbances in the morphology cannot be ruled out. A bar structure might be present, extending across the bulge, though it is not highly pronounced. Two main arms appear to dominate the structure of the galaxy, exhibiting distinct color gradients.
