NGC 424 emission line images from MUSE WFM (left), ALMA (middle), and the point-source subtracted MIRI MRS Ch3 medium (right). The images were obtained integrating the total [O III]λ5007, CO (2-1), and [Ne V] emission lines, respectively. Blue square in MUSE image represents the ALMA FoV considered in this work. Orange, red, yellow, and white rectangles in ALMA image represent the FoVs of MIRI MRS Channels 1, 2, 3, and 4, respectively. Black crosses mark the nucleus position, determined as the peak of Hα emission from the MUSE data. North is up and east is left.