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. Many of the small mineral grains consist of calcite or ferroan dolomite. The matrix appears to consist largely of iron-rich serpentine. The meteorite is a C2 chondrite. Traces of evaporite deposit are present.