This galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile is concentrated towards the center, with a gradual decrease in intensity outwards. It appears spheroidal in shape. There is no evidence of spiral arms or a prominent disk structure. There may be a very minor interaction or disturbance visible, but no merger is obviously apparent. The galaxy is relatively compact. The galaxy's color suggests an older stellar population and a low star formation rate. The dominant light is redder. Overall, the galaxy appears to be a quiescent system.
