The meteorite shows some well-defined chondrules and fragments dispersed in a recrystallized matrix. The best preserved chondrules are RP and BO and their sizes vary, mainly between 0.5 and 2.0 mm. The opaque phases are kamacite, taenite, troilite and tetrataenite. The latter is seen as a thin layer bordering taenite and plessite. Kamacite is mostly polycrystalline and in some cases plessite shows the pearlitic structure limited by tetrataenite. Sulphides are abundant and are present mainly as single grains. In some places small grains of plagioclase (partially isotropic) are observed. Some oxide veins, as well as iddingsite, penetrate the olivine fractures. A small amount of oxide is present around some metal grains. Melt Pockets are sparse and small. The olivine grains have edges with flat fractures, but clean nuclei, in which mosaic and / or wave extinction are weakly observed.