HD 90132 är en blå till vit stjärna i huvudserien av spektralklass A8 V. Den har en massa som är ca 1,7 solmassa, en radie som är ca 1,9 solradie och utsänder energi från dess fotosfär motsvarande ca 9,8 gånger solen vid en effektiv temperatur av ca 7700 K. Trots en låg ålder på 70 miljoner år har stjärnan en lägre ytgravitation än väntat. Detta beror på att radien vid ekvatorn är 18 procent större än polarradien, vilket i sin tur beror på en hög projicerad rotationshastighet på 270 km/s. Den har ett lätt underskott på metaller med en metallicitet på 74 procent av solens.
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