The object presents as a galaxy with a red shift, suggesting a relatively distant location. Morphologically, it is likely an elliptical galaxy. The galaxy exhibits a relatively smooth light distribution. The galaxy may be undergoing a merger, based on the possible disturbed morphology. The object displays an estimated effective radius of approximately 5.5 kiloparsecs. The luminosity is high, suggesting a massive system. The galaxy is a relatively quiescent system, with a low star formation rate.
