  We present a multi-wavelength study of the radio galaxy PKS J0334-3900, which
resides at the centre of Abell 3135. Using Australia Telescope Compact Array
(ATCA) observations at 1.4, 2.5, 4.6 & 8.6 GHz, we performed a detailed
analysis of PKS J0334-3900. The morphology and spectral indices give physical
parameters that constrain the dynamical history of the galaxy, which we use to
produce a simulation of PKS J0334-3900. This simulation shows that the
morphology can be generated by a wind in the intracluster medium (ICM), orbital
motion caused by a companion galaxy, and precession of the black hole (BH).
