The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. It is observed at an oblique angle, inclined relative to our line of sight, but not fully edge-on. Two tightly wound spiral arms are visible, emerging from a central bulge. The bulge displays a yellowish hue, potentially indicative of an older stellar population. The spiral arms exhibit a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. The spiral arms appear somewhat flocculent, with a patchy distribution of star-forming regions rather than a smooth, continuous structure. Overall, the morphology suggests a grand-design spiral galaxy experiencing active star formation within its spiral arms.
