Left: moment 0 maps of the CO (2–1) emission integrated over the velocity interval V_LSR = (−10, +3) km s⁻¹, highlighting the morphology of the blueshifted outflow lobe. The red contours at the center of the panel corresponds to the disk continuum emission at 1.3 mm drawn at [10, 200]σ_c, with σ_c=1.2×10⁻⁴ Jy beam⁻¹. The green square in the center of the contours marks the position of the continuum peak. The white dashed line at PA=48° indicates the orientation of the disk minor axis, and the white solid curves outline the spatial limits of the main wind components described in the text. Right: same as left panel, but with velocity integration range V_LSR = (+8, +30) km s⁻¹, illustrating the structure of the redshifted lobe. The beam is drawn in the bottom left corner. We note the difference in brightness between the two lobes: the blueshifted lobe is about ten times fainter.