The position of ESO 119-055 with respect to the star-forming main sequence. The gray shadow regions mark the scatter of data from the original papers, the best-fit lines were also present in the works cited below. Left panel: the main sequence sSFR versus M_* (S. Janowiecki et al. 2020), basing on the xGASS survey; the solid line is a main sequence with ±0.3 dex range (the dotted lines). At the right plot, the scaling relation is from E. Naluminsa et al. (2021) basing on the WHISP survey.