Wavelet-filtered absorption-corrected eROSITA surface brightness image restricted to areas with at least 1 ks exposure. Point sources have been excised. We note the apparent very long (~15 Mpc) continuous emission filament running from the Northern Clump through A3391 and A3395 down beyond the Little Southern Clump where cluster MCXC J0631.3-5610 lies outside the eROSITA FoV (its r₂₀₀ just visible at the bottom). There is an indication for an additional, weaker eastern filament. We also note the steep surface brightness gradients to the east and west of the 3 Mpc-wide emission bridge between A3391 and A3395. Emission from a few unrelated background clusters is also marked.