The galaxy presents a somewhat diffuse, but largely disk-like morphology. There is some evidence for spiral arm structure, but it appears loosely wound and ill-defined. A central bulge is discernible, though not highly pronounced; there is some asymmetry in the bulge region. There is a slight bar structure extending from the central bulge. Coloration suggests active star formation, particularly in regions along the spiral arms; these regions show a bluer tint. Dust lanes appear to be present, obscuring some regions. There is no evidence of a major merger event.
