The galaxy presents a distinct spiral morphology, with a clear disk structure. The arms are prominent and relatively tightly wound. There appears to be a moderate-sized bulge, contributing significantly to the central light concentration. The spiral arms exhibit a relatively high degree of symmetry, appearing to originate near the central bulge and extending outwards. The color gradient suggests a more evolved stellar population in the central bulge, indicated by the yellowish-orange hue, while the arms appear bluer, potentially indicating more recent star formation. There is a hint of a bar structure. No obvious major merging events appear to be occurring.
