Compact group SCG 0414−5559. Left panel: colour composite VST image of the Dorado group centre (north is on the top and east is to the left). The field of view is 5177 × 4752. The SCG is at the centre of the Dorado members’ velocity distribution in the Kourkchi & Tully (2017) group definition (central panel). The colour RGB image is created adopting the Lupton et al. (2004) scheme, using the r-band image as R channel input, the g-band as B channel input, and the average image between r- and g-bands as G channel input. We notice faint shell and/or ripple structures in NGC 1549 and NGC 1553 (see Malin & Carter 1983) and in the south-east side of NGC 1546. In the right panel, an unsharp mask of the SCG is shown. In red is drawn the circle that encloses the compact group, SCG 0414−5559, identified by Iovino (2002, see her Fig. 3 and Table 1). In addition to galaxies forming the compact group, we labelled PGC 75125, a physical companion of IC 2058 (see e.g., Elagali et al. 2019) and CMI2001, not present in Iovino (2002). Our B, C, D, and E UVIT fields are superposed on the unsharp masking of the g-band VST image in order to show the extension and distribution of the FUV emission within the compact group members.