Overview of NGC 4593’s host galaxy on different spatial scales. Optical imaging from PanSTARRS gri colour (top left) shows the spiral host of NGC 4593 with a the 9.1 kpc dominant bar. A zoom-in of the HST/WFC3 F547M image shows the prominent dust lanes connecting the dust lanes of the bar with a nuclear single-arm spiral. The MUSE WFM FOV (top centre) covers 1′ × 1′ of the dominant bar. UV imaging from HST/ACS HRC covers the inner 29′′ × 26′′. The right panels show the moment 0 map of the ALMA CO(2−1) data combining data taken in two different configurations and covering the innermost 26′′ at a resolution of up to 40 mas.