The galaxy presents as a singular, luminous structure, exhibiting an elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center, suggesting an older stellar population. Color analysis indicates a redder hue, potentially indicative of evolved stars and a lower rate of ongoing star formation. There is a possible faint extended halo of light surrounding the core of the galaxy. Close inspection suggests that the object might be undergoing a merger. The galaxy does not have any distinct spiral arm structures. Overall, the galaxy appears to be a large, relatively quiescent system, observed at a redshift which places it at a considerable cosmological distance.
