This galaxy presents as a spiral, observed at an angle approaching face-on. Multiple spiral arms are discernible, exhibiting a moderate winding pattern. The arms display subtle color variations, hinting at differing stellar populations or dust lane presence. The central bulge appears relatively small and not highly pronounced, displaying a yellow-orange hue, indicative of an older stellar population. The overall structure suggests a galaxy that is not strongly barred. There may be a slight disturbance in the outer disk region suggesting minor interactions.
