Here's the nodal precession due to the short-periodic perturbations on the
osculating ascending node.
The two vertical dashed lines represent the orbital period.
The linear regression shows an average precession rate of 0.7 deg/minute or 1.008 deg/day. The epoch of the TLE is 18309.94944316 (Nov 5) and for that epoch, the Earth's angular speed around the Sun was 1.003 deg/day (result obtained from the JPL's DE430 ephemerides), hence the satellite is almost exactly in a Sun-synchronous orbit (please, see
here for the details, select "AQUA" and
here).
Like the previous graph, also this graph shows the short-periodic perturbations, but this graph is for the inclination.
The largest perturbation in the inclination is 0.0052 deg and its period is half the orbital period.
The largest perturbation in the semi-major axis is 9 km and its period is half the orbital period.