  The stationary axisymmetric spacetime coupled to nonlinear Born-Infeld
electrodynamics is studied. The solution was derived by Plebanski et al (1984)
and it is characterized by six free parameters: mass, NUT charge, electric and
magnetic charge, Born-Infeld parameter and cosmological constant. The geodesic
and Lorentz force equations are integrated, and a qualitative analysis of the
effect of varying the parameters in the effective potential is provided. Then
the light and charged particle trajectories are discussed. The conditions that
determine an extreme black hole are presented as well.
