The galaxy presents as a relatively smooth, elongated structure with a prominent central bulge. Its light profile appears centrally concentrated, lacking distinct spiral arms or other complex features. The overall color is redder, suggesting an older stellar population with lower rates of recent star formation. There is a possibility that it is either undergoing or recently underwent a minor merger, but there is not enough strong evidence for either. The morphology suggests a galaxy transitioning towards an elliptical form. 
