  We derive the multipole moments of the Kerr-NUT black hole spacetime using
the Geroch-Hansen formalism, even though the spacetime is not asymptotically
flat. Intriguingly, in the presence of the NUT charge, the absence of
reflection symmetry about the equatorial plane, leads to mass and spin
multipole moments of all orders, in stark contrast to Kerr-like spacetimes.
This leads to a drastic departure of the multipolar structure of a compact
object with NUT charge, whose implications for gravitational wave observations
have been explored. Our analysis of multipole moments for the Kerr-NUT
spacetime is also in tune with the Thorne's approach.
