As noted in the answer by Michael, a precise chemical composition is not known at this time.
We can, however, consider the overall mineral composition on the surface of the Gale Crater. This diagram provided by Curiosity's CheMin analyzer (source) shows that the composition varies with depth inside the crater:

The lower part of the crater contains large amounts of magnetite, $\text{Fe}_3\text{O}_4$ and mafic minerals, the latter being silicates rich in magnesium, iron and calcium (magnesium+ferrum+ic). Under weathering conditions with water and an oxidizing atmosphere, such as might have existed in earlier Martian history, the magnetite would be oxidized to hematite ($\text{Fe}_2\text{O}_3$), which is seen in the upper regions in preference over magnetite. The mafic minerals would be decomposed, a process known also on Earth (where the most common igneous rocks exposed on the surface, such as granite, are felsic rather than mafic). This weathering can lead to various products such as more iron oxides (which again would be oxidized to hematite), lighter silicates such as feldspar and clay, silica ($\text{SiO}_2$), and perhaps salts of the calcium and magnesium depending on other materials and environmental conditions. Thus the composition difference between lower and upper regions appears to be due to the upper regions being weathered while the lower regions, perhaps protected until the atmosphere became thinner, is more "preserved".
In the presence of sulfur-bearing materials the weathering of mafic minerals could indeed form calcium sulfate, therefore the gypsum ($\text{CaSO}_4\cdot 2\text{H}_2\text{O}$) or anhydrite ($\text{CaSO}_4$, no included water); both of these minerals may appear translucent. Like hematite and the lighter silicates, calcium sulfate is concentrated in the weathered upper regions and not in the mafic/magnetite-rich lower regions. Thus gypsum or anhydrite is one possibility for the material in question, most likely if the image is from the upper part of the crater.