Houk and Swift (1999) found a class of G8IV, suggesting it is instead a more evolved subgiant star. It is around seven billion years old and is spinning slowly with a projected rotational velocity of 1.5 km/s.
Houk and Swift (1999) found a class of G8IV, indicating it might be an advanced stage subgiant. It is estimated to be about seven billion years old and rotates at a relatively slow pace with a velocity of 1.5 km/s.