The galaxy exhibits a clear spiral structure, with prominent arms extending outwards from a central bulge. These arms are not tightly wound, appearing more open and grand design. The color of the spiral arms appears bluish, suggesting ongoing star formation. The central bulge is relatively small and has a yellow-orange hue, indicative of an older stellar population. The galaxy appears to be mostly face-on. There is no evidence of a strong central bar. A slight warp is visible in one of the spiral arms. There is no large disturbance indicating an ongoing merger.
