The galaxy presents a morphology consistent with a spiral galaxy, exhibiting a disk structure. While the image resolution limits detailed observations, there's a clear indication of spiral arm structures extending from a central bulge. These spiral arms appear relatively tightly wound and possess a mottled texture. The color gradient suggests some active star formation regions, particularly along the spiral arms. The bulge appears prominent, transitioning smoothly into the surrounding disk, indicating an intermediate bulge classification. Overall, the galaxy shows little evidence of any recent major merging event, appearing relatively undisturbed.
