Another neat point about this is that for habitable gas giants, the Laplace radius could be within the range of orbital distances of the satellite system. E.g. for Jupiter at 1 AU around a solar-mass star, the Laplace radius would be roughly between the orbital distances of Europa and Ganymede.
Outer moons would therefore be better aligned with the planet's orbit than the planet's equator (similar to our own moon), and therefore if the planet has significant obliquity and had a ring system you'd get a good view of the rings from the moon. On the other hand you wouldn't have seasons unless the planet's orbit is substantially eccentric.