Axis-ratio histograms ( df/ dq _proj) of early-type galaxies with all masses log( M/ M _☉) > 10.7 (our full sample) as a function of redshift in bottom three panels, always compared with the present-day sample from H12. The top panel shows cumulative histograms for all redshift bins as a function of projected axis ratio f(< q _proj). Up to z = 0.8, as confirmed by the M-W statistical test (of which the probability is given that the samples are statistically the same), there is no significant redshift evolution in the projected axis-ratio distribution, consistent with the results from H12. At z > 1, we find that early-type galaxies are flatter than their present-day counterparts.