Fraction of strongly bulge-dominated early-type galaxies (n ≥ 3) as a function of the distance from the BCG (top) and the distance from two quasars (one quasar at z = 2.236, and the other at z = 2.229; bottom). The quiescent BCG and the two quasars are ∼1 Mpc apart. In both cases, we found a peak in the distribution of n ≥ 3 bulge dominated galaxies near the target galaxy, with the BCG showing a less steep distribution.