Side-on rendering of the galactic disk after t = 250 Myr. Comparing the effect of resolution on the early evolution of the galaxy. Left to right goes from low to high resolution Top panel show density, middle panel magnetic field strength and bottom panel the toroidal magnetic field. The increase in resolution show additional the CGM. Feedback leads to the formation of an interesting vertical structure of the magnetic field, where near the central disk, we can see plenty of reversals and intricate behaviors in the magnetic field. The complexity of the structure around the central disk increases as we increase the resolution. The outer regions can be seen to be dominated by the blowout of the initial magnetic flux.