The galaxy presents as a face-on spiral, with a pronounced central bulge. The bulge exhibits a yellow-orange hue, suggestive of an older stellar population. Surrounding the bulge, discernible spiral arms extend outwards, displaying a patchy blue-green color. These arms may indicate regions of ongoing star formation. The spiral arms appear moderately wound, presenting an intermediate structure between tightly wound and loose, flocculent arms. There is a suggestion of multiple arms, although a precise count is difficult to ascertain. A possible bar-like structure is oriented along the horizontal axis of the image, though its strength and extent are somewhat ambiguous. Overall, the galaxy demonstrates a relatively normal spiral morphology, without any obvious signs of major interactions or disturbances, though minor disturbances cannot be ruled out.
