Just because the dataset has gaps does not mean it is worthless... even if we only see a few planets, or a few types of planet, or that our detection equipment has limitations, does not stop this knowledge from adding to the picture of planetology in general.
But our detection methods are biased, particularly towards large planets close in to their stars.
Also, keep in mind that all we've found so far is balls of lava, balls of ice, and balls of gas. Nothing even remotely habitable by terrestrial standards.
That's not true. Those are extremes, we've found other planets that fall in the middle. We've found planets that, while they are hardly Earth-analogues, don't fit those stereotypes.
And our detection methods have large biases. There are likely many 'genres' of planet out there that we aren't able to detect yet, or detect usefully.
One thing that our solar system has taught us though, is that there are many ways to be a planet and not be much like Earth at all.
So even if you want to jump to conclusions from the probably non-representative sample from Kepler, the obvious conclusion to jump to would be that yes, we are in fact alone.
If you want to call "I wish and hope that aliens do not exist" "jumping to conclusions", then yes, that would be a good conclusion to jump to.
Currently the only conclusion I personally can 'jump' to, is that the most likely biased, and incomplete sample presents some results that people didn't quite think about before, that could be the result of interesting phenomena that could teach us more about the bigger picture.