NGC 4349-127 is a probable red giant star approximately 6,100 light-years away in the constellation of Crux.
[4] Its mass is estimated at 3.9 times Solar, and its age is about 200 million years.
It orbits its host star at a distance of 2.38 AU in a period of 677.8 days.
This object was discovered by Christophe Lovis and Michel Mayor of the Geneva Observatory using the radial velocity technique.
[3] A 2024 study also found the radial velocity signal to be caused by non-radial oscillations.