The galaxy presents as a somewhat elliptical, unresolved object at a considerable distance. Its core region exhibits a high degree of luminosity, suggesting a dense concentration of stars, or possibly AGN activity, although the available image resolution does not allow for conclusive determination. There are no discernible spiral arms or disk-like features, which is consistent with it potentially being an elliptical or lenticular galaxy. Faint blueish emissions are observed surrounding the central yellowish core. This likely denotes lower levels of recent star formation, although overall the galaxy appears to be relatively quiescent. The overall structure appears mostly undisturbed; there are no obvious signs of ongoing or recent major merger events. 
