The galaxy presents as a relatively compact object with a smooth, somewhat rounded morphology, although some features may be present. The galaxy appears to be mostly smooth, but there is evidence of some substructure within the galaxy. It shows a slight deviation from perfect circularity, leaning more towards an in-between, disc shape. There is no strong visual indication of a major ongoing merger, though minor disturbances within the galaxy cannot be ruled out. The overall color of the galaxy appears blue, which could indicate a relatively younger stellar population and ongoing star formation, but it also appears to have a high redshift which would indicate an older galaxy. 
