Recent studies of galaxy rotation directions in the distant universe have confirmed the observed trend for an asymmetry of up to 50% more counter rotating galaxies than co rotating galaxies. In that there appear to be more galaxies that rotate counter to our Milky Way than with it. These observations are currently not consistent with the Big Bang theory. And suggests new models of the physics of galaxy rotations may be necessary. Here it is proposed one can use the differing amounts of aberration of light from co and counter rotating galaxies to explain this apparent asymmetry. In that light from co rotating galaxies arrives at the earth observer more dispersed or blurred than light from counter rotating galaxies. Making the rotation direction of co rotating galaxies harder to identify. And in turn creating an asymmetrical bias in the identification between co and counter rotating galaxies. A counter rotating galaxy will appear more sharply in focus and more easily identifiable than the more blurred co rotating galaxy at any similar redshift. And that this asymmetrical bias due to aberration and the relative differences in incident angles between light from co and counter rotating galaxies increases with higher redshifts.