The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution with a slightly elongated shape. There is evidence of possible minor disturbances in the morphology, perhaps indicating an ongoing or recent interaction. The light profile appears generally uniform, with a concentrated central region exhibiting a yellowish-red hue. The galaxy has a significant red shift, suggesting that it is a moderately distant galaxy. The object is likely a high mass galaxy that is undergoing some star formation.
