The galaxy exhibits a morphology consistent with a spiral galaxy classification. It is observed nearly face-on, presenting a flattened disk structure. The disk component dominates the overall appearance. The spiral arms appear tightly wound, displaying a coherent, organized pattern emanating from the central region. A substantial bulge is readily apparent, exhibiting a moderate size relative to the galactic disk. A bar structure may be present, though its features seem unclear, and thus its presence cannot be reliably confirmed. There is no indication of major mergers or significant tidal disturbances. The central region of the galaxy appears yellow-white, suggesting an older stellar population, while the outer spiral arms display a bluer hue, indicative of ongoing star formation.
