The galaxy presents a clear spiral structure, with two prominent arms extending from a central bulge. The spiral arms appear loosely wound. The color gradient suggests active star formation within these arms, evidenced by their bluer hues, while the bulge exhibits a yellowish tint, potentially indicating an older stellar population. The galaxy displays some degree of asymmetry, possibly resulting from minor gravitational interactions. There is some evidence of disturbance in the disk. The bulge appears of moderate size, with no signs of strong barred structure. Overall, it appears to be a relatively massive spiral galaxy undergoing active star formation within its arms.
