Panel a) the continuum emission at 150 MHz as detected with LOFAR, with contours at −3, 3, 5, 10, 20, 40, 60, 80, 100, 120, 140, 200, 250, 300] × 0.15 mJy beam^-1 plotted in white in darker areas and black in brighter areas. The CLEAN restoring beam of , position angle 161°, is plotted as a solid red ellipse in the lower left. Positions are relative to RA , Dec . The black dots in the centre mark the 33 GHz continuum positions of the two nuclei (Barcos-Muñoz et al. 2015) with radius 133 mas illustrating the total maximum astrometric uncertainty between the 150 MHz (83 mas) and 33 GHz (50 mas). Panel b) a sketch of the structure discussed in this paper. The labels mark the extended kpc-scale disk, the outflows from the east and west nuclei (small ellipses), the large scale outflow and the north-west and south-east “hooks”. The blue triangles represent the closer sides of outflows and the red triangles the far sides.