See the feature article on oxygen-poor galaxies in the https://www.skyandtelescope.com/sky-and-telescope-magazine/inside-april-2018-issue/ issue of Sky & Telescope.
The dust-to-gas ratio varies with the metallicity of a galaxy. For giant galaxies, like the Milky Way, the dust-to-gas ratio is on the order of 1%. For the Magellanic Clouds, which are smaller than the Milky Way and thus more metal-poor, the dust-to-gas ratio is lower. And for the most metal-poor galaxies, such as I Zwicky 18, the dust-to-gas ratio is roughly 0.001%, as stated in the Sky & Telescope article, which also includes a color image of the galaxy. Note, though, that this percentage is somewhat uncertain.