CO(2–1) channel maps from +115 km s⁻¹ to +190 km s⁻¹ (step of 15 km s⁻¹; projected velocities) relative to a systemic velocity of v_sys = 3568 ± 7 km s⁻¹ (this work). A complex filamentary emission in a gradually denser ISM is revealed within the outflowing wind, starting with a diffuse emission trail at , (black arrow; projected distance of 340 pc from the AGN) followed by a jet-ISM impact point at , (pink marker; projected 440 pc). After the bifurcation, the wind expands and develops a cone-like structure where the highest velocities are found along its central axis. The solid green contours correspond to the integrated [Ne II]_12.8μm emission from VLT/VISIR (starting from 3× RMS with a spacing of ×10^N/4). The black star indicates the position of the AGN in the 1.2 mm continuum map. The synthesised beam size is shown in the lower right corner of the first panel.