Velocity (left) and dispersion (right) maps of the ionised gas derived from the Fabry-Perot data. The black box indicates the region covered by the MUSE exposure. The red contours show the VESTIGE Hα surface brightness at 3 × 10⁻¹⁷ erg s⁻¹ cm⁻² arcsec⁻². The white cross, star, and filled circle show the position of the photometric, stellar, and gas kinematical centres, respectively. As for the previous figures, the velocity of the gas is given relative to the systemic velocity of the galaxy of −170 km s⁻¹.