They show scattered chondrules, up to 0.6 mm across, a few irregular aggregates, and small mineral grains in a dark brown to black matrix. The minerals are almost entirely olivine near Mg2SiO4 in composition, with a few more iron-rich grains. A little pyroxene near MgSiO3 in composition is present. The matrix appears to consist largely of iron-rich serpentine. The meteorites are a C2 chondrites.
Flow marks are present on all surfaces.
Evaporite deposit is present immediately underneath the fusion crust. The section shows a few chondrules, up to 0.7 mm across, and numerous small mineral grains in a dark brown to black matrix. Some chondrules consist of granular or porphyritic olivine, but most have been converted to brown serpentine. Fusion crust is present along one edge. Olivine is near Mg2SiO4 in composition, with a few more iron-rich grains.