The formal explanation of the answers above is as follows. Take an arbitrary volume ##V## with boundary ##\partial V## out of a fluid. Then there's a force corresponding to the interaction of the fluid outside of the volume on the surface of the volume. The total force (neglecting bulk forces like gravity) on the fluid volume then is given by
$$F_j=\int_{\partial V} \mathrm{d}^2 f_k \sigma_{kj},$$
where ##\sigma_{kj}## is the stress tensor of the fluid and ##\mathrm{d}^2 \vec{f}## the surface-normal vectors along the boundary of the volume pointing by convention outward of the volume.
Pressure is one part of the stress tensor of a fluid
$$\sigma_{jk}=s_{jk}-P \delta_{jk}.$$
By definition ##s_{jk}##, the "stress deviator", is traceless and thus
$$\sigma_{jj}=-3 P$$
Since ##\sigma_{jk}## is a 2nd rank tensor, the pressure is a scalar.
The geometrical meaning is that the pressure tries to change the magnitude of the volume, while the traceless stress deviator tends to deform it.
The Wikipedia article on this topic is very nice with very good figures, making the thing pretty intuitive:
http://en.wikipedia.org/wiki/Cauchy_stress_tensor