The galaxy appears as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a dominant bulge component, as there is no clearly defined spiral arm structure or significant dust lane obscuration visible. There is a slight elongation of the galaxy's shape. The color profile indicates a gradual shift from bluer hues in the outer regions to a somewhat redder color towards the central bulge, suggesting a difference in stellar populations or dust content. Overall the structure is largely undisturbed with only small signs of a possible minor merging event. 
