  In galaxy cluster collisions, the gas can be separated from dark matter
halos. Abell~56 displays signatures of a dissociative bullet-like merger with a
possible high inclination angle between the plane of orbit and the sky. Our
objective is to provide a comprehensive description of the features observed in
the collision scenario of Abell~56. Additionally, we aim to apply a potential
weak lensing mass bias correction attributed to the merger to evaluate its
impact on our findings. To investigate this, we perform tailored hydrodynamical
$N$-body simulations, varying the impact parameter. We initially identified an
early scenario at $0.12$\,Gyr after the central passage that reproduces some
observational features. However, the mean temperature of $9.7$\,keV exceeded
the observed value. Our best model corresponds to the late scenario at
$0.52$\,Gyr after the pericenter, reproducing observed features of Abell~56,
with an inclination of $58^\circ$. These features include the offset of
$103$\,kpc between the main gas density peak and the south dark matter density
peak, gas morphology, a line of sight relative velocity of $184$\,km\,s$^{-1}$,
and a mean temperature of $6.7$\,keV. This late model provides a plausible
scenario to describe the dynamics of Abell~56. The weak lensing mass bias did
not significantly impact the overall dynamics of this cluster merger.
