The galaxy presents as an elliptical morphology with a smooth light profile. There is a prominent central bulge that appears slightly more concentrated in luminosity. Color gradients suggest a stellar population of intermediate age, with a possible ongoing but low level of star formation based on the relatively bluer color compared to other ellipticals. No obvious spiral arm structures or dust lanes are apparent. The overall structure suggests a relatively undisturbed system. The red shift indicates the galaxy is at a considerable distance. The galaxy is not interacting or merging with any other galaxies nearby.
