Disk galaxies form as a consequence of the existence of a non-vanishing tidal field at the time the gravitational collapse of the galaxy decouples it from expansion. This is a good reference if you want to read the details at early epochs of this process. But, as you mention, it boils down to conservation of angular momentum. These galaxies are said to be supported by rotation, in the sense that the rotation velocity dominates the random motion, in other words the number $V_{\rm circ}/\sigma$ is large.
The problem is that kinematic cold disks are in general very unstable, and even small perturbation over time can destroy them, ending up in galaxies with more spherical shapes. Evolution in a hierarchical universe, such as ours, will naturally lead to young disk galaxies and old elliptical galaxies. Although this is still a matter of debate.
This argument should also give you an idea as to why there are no disk stars: at the time of formation, material indeed can be accreated in the shape of a disk, but over time, all the instabilities generated by the formation of the star would relax the system to a spherical shape