Hi Darkan9el, welcome to PF!
When we talk about the rotation of a rigid body, like a planet, it's easy to say where the axis of rotation is located, as no matter which point on or inside the planet you choose, it will rotate around the same axis.
With solar system, it's a bit more complicated, as the particles(i.e., planets, asteroids, the Sun, comets, gas) comprising the system are not rigidly bound together, so they can move in orbits whose axes of rotation each point somewhere else.
It is thus impossible to name a single axis that would fit all the celestial objects.
However, due to the dynamics of the formation of the solar system, all planets ended up orbiting in nearly the same orbital plane, very close to that of the Earth. As a first approximation then, it's possible to say something like "the line perpendicular to the ecliptic(Earth's orbital plane) passing through the Sun is approximately the axis around which most objects in the solar system orbit".
Such an axis points towards the constellation Draco, pretty much in the centre of the first loop of the Dragon's serpentine body, counting from the head. There are no particularly bright stars there. The star Polaris is, unsurprisingly, 23.5 degrees away from this point.
A bit better, more rigorous approach would be to calculate the total angular momentum of the solar system, by adding component vectors from each of the major bodies(Sun, planets) in the system. The direction of the resultant vector wouldn't differ from the previous approach by more than a few degrees, though.