The galaxy presents an overall elliptical morphology with a smooth light distribution, with a hint of a disc structure. The core region exhibits a high surface brightness and a relatively round shape. The outer regions display a gradual decline in luminosity. The main body of the galaxy is estimated to be a few kiloparsecs in radius. There's a hint of some disturbance in the galaxy. Overall the galaxy is a fairly massive object with a low star formation rate. The object is located at a significant cosmological distance.
