The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. Its color index, apparent from the color image, indicates a prominence of older stellar populations, and its high inferred stellar mass indicates that it is likely a large galaxy. It has a significant level of smoothness which may indicate an elliptical galaxy type. There does not appear to be any evidence of any distinct spiral arms. Furthermore, there are no signs of any major mergers occuring, or any significant tidal features or distortions that would be associated with such an event. 
