The galaxy presents as a spiral type, exhibiting a distinct disk structure. Two prominent spiral arms are readily observable, loosely wound around the central bulge. There is evidence of a bar-like structure spanning the central region of the galaxy. The bulge appears to be of moderate size, and there is no clear signs of an ongoing major merger event. The general color profile of the galaxy shifts from a yellow hue at the bulge to a more blue-ish tinge in the outer disk. There is evidence of star formation occuring in the outer disk due to the blueish tint in the disk, suggesting the presence of hot, young stars in the spiral arms.
