  The Bardeen solution corresponding to Einstein field equations with a
cosmological constant is a regular black hole. The main goal of this manuscript
is to investigate the geometric structures in terms of curvature conditions
admitted by this spacetime. It is found that this spacetime is pseudosymmetric
and possess several kinds of pseudosymmetries. Also, it is a manifold of
pseudosymmetry Weyl curvature and the difference tensor C.R-R.C linearly
depends on the tensors Q(g;C) and Q(S;C). It is interesting to note that such a
spacetime is weakly generalized recurrent manifold and satisfies special
recurrent like structure. Further, it is an Einstein manifold of level 2 and
Roter type. The energy momentum tensor of this spacetime is pseudosymmetric and
finally a worthy comparison between the geometric properties of Bardeen
spacetime and Reissner-Nordstr\"om spacetime is given.
