Venus actually rotates west to east, very slowly. Its year is shorter than its day.
Uranus rotates nearly 90 degrees in relation to the ecliptic.
Mercury rotates east to west, but has a special orbital resonance with Earth. Because its so close to the sun, for decades we could only see it well enough at certain points in its orbit. Because of the resonance, we basically always see the same face which made it appear to be tidally locked. It rotates quite fine, but it wasn't until the last couple of decades of sending probes by Mercury that its rotation could actually be detected.
There's just 3 examples in our own real solar system that disprove the "convention". Not even to mention the hundreds to thousands of other smaller bodies that are unique in their own ways.
Given that: how do you define what rotational-pole is "north", to derive east/west? Or is it not based on a planet's qualities, in which case it's likely something solar, and then what would Uranus' "north" (or east) be?
For relatively perpendicular though, yeah - that largely works I think. But then we should expect most to be "sun rises in the east" as, as far as I'm aware, most solar system bodies orbit and rotate in the same direction as their star does.
edit: perhaps from directly above the equator you would still consider the spin to be clockwise or anticlockwise -- but which one would depend on your orientation.
Using the elliptic plane is a fine answer, but is just a convention.
Is there a different definition of determining a planet’s east/west side?
Seems odd to call that a blunder, surely that's just a matter of convention?