Same as Fig. 4, but with mid-inclined orbits relative to the equatorial plane of the black hole. We see that that the apocenter experiences both an in-plane and out-of-plane precession due to the LT effect. The in-plane precession is clockwise as seen on the face-on projection of Fig. 4a, and the out-of-plane precession is mainly for the major axis but also acts on the minor axis. We also see that the quadrupole moment appears to have the opposite behavior to the LT effect for both the in-plane and out-of-plane shifts.