HD 88133 is a yellow star with an orbiting exoplanet in the equatorial constellation of Leo.
It has an apparent visual magnitude of 8.01,[2] which is too faint to be visible to the naked eye.
The distance to this system, as measured through parallax, is 240 light years, but it is slowly drifting closer with a radial velocity of −3.6 km/s.
[4] This is classified as an ordinary G-type main-sequence star with a stellar classification of G8V.
[3] However, D. A. Fischer and associates in 2005 listed a class of G5 IV, suggesting it is instead a subgiant star that is evolving away from the main sequence having exhausted the hydrogen at its core.