The galaxy presents as a relatively well-defined spiral structure. The arms appear somewhat tightly wound around a central bulge that seems relatively small in proportion to the overall disk size. The galaxy is viewed from a near-face-on orientation. There are multiple spiral arms. The central bulge appears yellowish-white in color, and the spiral arms exhibit a bluer hue, suggesting ongoing or recent star formation activity within the disk. There is some indication of dust lanes within the spiral arms, particularly in the inner regions. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger event, although minor irregularities or disturbances cannot be ruled out based on this image alone. There is an indication of a bar-like structure in the center of the galaxy.
