The galaxy presents as a spiral with a prominent central bulge. The bulge appears yellow-white, suggesting an older stellar population. Spiral arms are visible, although somewhat tightly wound and not sharply defined. They exhibit a bluer hue than the central bulge, consistent with ongoing star formation. A possible bar structure is seen crossing the central bulge, though it's not sharply defined. The overall morphology suggests the galaxy is a late-type spiral, exhibiting a significant disk component. It shows no major signs of recent mergers, though there is a suggestion of some disturbances in the disk's structure, potentially indicating a minor interaction or internal dynamics. The galaxy is neither perfectly face-on nor edge-on, displaying an intermediate inclination.
