Stellar velocity field, stellar rotation model, residual velocity field (observed – model), stellar velocity dispersion (all in units of km s⁻¹ following the colour bars above panels), and the structure map (the bright nucleus masked to show details better at fainter fluxes) for ESO 362-G18. In the left panel the solid (dashed) black line indicates the position of the kinematic major (minor) axis. The cross denotes the continuum peak in all panels.