The galaxy presents as a spiral, observed at an oblique angle, but not fully edge-on. The central bulge appears prominent and has a yellowish color, suggesting a population of older stars.  Spiral arms are present, though somewhat ill-defined in the image. The disk shows mottled blue regions, indicative of star formation. There are some signs of minor disturbances within the arm structures. The winding of these arms can be classified as somewhere between medium and loose. There is no strong evidence of a bar structure in the central region. The overall morphology suggests this galaxy is not currently undergoing a major merger.
