  We discuss the generalization of the NUT spacetime in General Relativity (GR)
within the framework of the (dynamical) Einstein--Chern-Simons (ECS) theory
with a massless scalar field. These configurations approach asymptotically the
NUT spacetime and are characterized by the `electric' and `magnetic' mass
parameters and a scalar `charge'. The solutions are found both analytically and
numerically. The analytical approach is perturbative around the Einstein
gravity background. Our results indicate that the ECS configurations share all
basic properties of the NUT spacetime in GR. However, when considering the
solutions inside the event horizon, we find that in contrast to the GR case,
the spacetime curvature grows (apparently) without bound.
