HD 101782 är en röd till orange jättestjärna av spektralklass K0 III, som anger den som en utvecklad röd jätte, som för närvarande befinner sig på den horisontella jättegrenen och genererar energi genom kärnfusion av helium i dess kärna. Den har en massa som är ca 2 solmassor, en radie som är ca 10 solradier och har ca 55 gånger solens utstrålning av energi från dess fotosfär vid en effektiv temperatur av ca 4700 K.
TYC 9507-3649-1 är en optisk följeslagare av 10:e magnituden som ligger med en separation av 25,9 bågsekunder vid en positionsvinkel av 139°. Denna följeslagare upptäcktes 1837 av astronomen John Herschel.
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