  We report the discovery of a secondary pair of radio lobes in the Seyfert
galaxy NGC 2639 with polarization-sensitive observations with the Karl G.
Jansky Very Large Array (VLA). The presence of these lobes, which are aligned
nearly perpendicular to the known set of radio lobes observed in the east-west
direction, has not been reported previously in the literature. The in-band
rotation measure image shows gradients in both the lobes indicative of
organised magnetic field structures on kpc-scales. The magnetic field structure
is aligned with the jet/lobe direction in both the lobes. Based on the settled
optical morphology of the host galaxy, it is likely that a minor merger that
did not disrupt the host galaxy structure is responsible for the observed
features in NGC 2639. This also explains the near 90$^o$ change in the jet
direction; the current jet direction being the result of a new accretion disk
formed by the minor merger, whose direction was a result of the angular
momentum of the inflowing merger gas.
