Multi-wavelength view of UDG 32 and its environment. From left to right: VST OmegaCAM g-band image (Iodice et al. 2021) of UDG 32 and NGC 3314A/B with black contours tracing the H I emission detected by the MeerKAT survey (Hess et al. 2022), VST OmegaCAM colour-composite image (Iodice et al. 2021) with the location of UDG 32 highlighted by the orange box, colour-composite derived from the MUSE data presented in this paper, and MUSE white-light image with the Hα emission overplotted by the blue colour map. The dashed ellipse denotes the 1 R_eff isophote of UDG 32 derived by Iodice et al. (2021) and the purple circles the two intracluster GCs that were spectroscopically confirmed in this work. The orange circle denotes the aperture from which we extract the spectrum to derive the LOS velocity of UDG 32. Coordinates in this and all following figures are in J2000.0, and North is up and East to left.