The crater has a symmetrical bowl-shaped topography and is considered to be one of the best preserved small meteorite craters on Earth. The 20 m wide rim rises about 1.5 m above the plain, while the deepest point of the central depression is 7 m below the rim crest; the rim to rim diameter averages about 70 m. Based on cosmogenic nuclide exposure dating of the crater walls, the crater is less than 20 thousand years old, while the pristine state of preservation of the ejecta has been used to suggest that it may in fact be less than 4 thousand years old.
The iron meteorite fragments collected around the crater are classified as a coarse octahedrite belonging to chemical class IIAB; the fragments show considerable evidence of deformation presumably related to the impact explosion. It has been inferred that the original meteorite was in the size range of 100-1000 tonnes, probably closer to the latter, now dispersed as fragments within the crater filling breccia and ejecta.