Multifrequency images of NGC 4330 at their intrinsic resolution. From the top left to the bottom right: CFHT/VESTIGE Hα, GALEX FUV, CFHT/NGVS u*, CFHT/VESTIGE r, Spitzer/IRAC 3.6 μm, and Herschel/PACS 100 μm. All the images are on the same scale and are oriented such that north is up and east is left. The red contours are drawn from the r-band image at the 22nd, 23rd, and 25th mag arcsec⁻² and clearly highlight the different amount of disc truncation at different wavelengths. The presence of a tail extending to the SW is clear in the FUV image.