The crater has a symmetrical bowl-shaped topography and is considered to be one of the best preserved small meteorite craters on Earth. Abstract The wide rim rises about above the plain, while the deepest point of the central depression is below the rim crest; the rim to rim diameter averages about . 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.
