Gamma Crateris is a binary star[7] system, divisible with a small amateur telescope,[14] and located at the center of the southern constellation of Crater.

[2] With an annual parallax shift of 39.62 mas as seen from Earth, this star is located 82.3 light years from the Sun.

[15] The star was confirmed by Gabriel Cristian Neagu and Jan Ovidiu Tercu as a variable of DSCT type.

[12] The primary is radiating 18.8[9] times the solar luminosity from its outer atmosphere at an effective temperature of 8,020 K.[10] Based upon the detection of an infrared excess, the star may host an orbiting debris disk.

As of 2010, the companion was located at an angular separation of 4.98 arc seconds along a position angle of 93.1° relative to the primary.