The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of central brightness that decreases gradually toward the outer regions. There is a subtle colour gradient observed, with the central region appearing more yellow/white, suggesting an older stellar population. The outer regions show a hint of blue, which could indicate ongoing star formation or a younger stellar population. The lack of distinct spiral arms or a prominent disk structure supports its classification as an elliptical galaxy. The overall morphology appears undisturbed, with no signs of significant tidal features or recent merger events.