The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology with a dominant, round central bulge. Evidence suggests that the galaxy is undergoing or has recently undergone a merger, due to the disturbed morphology with signs of tidal features or a potential companion galaxy.

The galaxy is luminous with a magnitude indicating a significant mass. The galaxy's color index suggests a population of older stars with relatively little ongoing star formation. The galaxy exhibits low star formation rate and specific star formation rate.

