Results of new polarimetric observations of the magnetic white dwarf G
D 229 carried out in 1994 are reported. A comparison of these results
with previously published results has revealed long-term variations in
the linear and circular polarization on a time scale of similar to 10
yr. To interpret this variability, two fundamental possibilities are
explored: very slow axial rotation and precession. Based on an analysi
s of the polarimetric data for GD 229, we have obtained an approximate
estimate of the period of the variations. This period is shown to be
greater than or equal to 80 yr.