  In this paper we study cosmological dynamics of phantom as well as
non-phantom fields with linear potential in presence of Galileon correction
$(\partial_\mu\phi \partial^\mu\phi) \Box \phi$. We show that the Big Crunch
singularity is delayed compared to the standard case; the delay crucially
depends upon the strength of Galileon correction. As for the phantom Galileon,
$\rho_{\phi}$ is shown to grow more slowly compared to the standard phantom
delaying the approach to singularity. In case, $V\sim \phi^n, n>4$, Big Rip is
also delayed, similar phenomenon is shown to take place for potentials steeper
than the exponential.
