The galaxy presents as a smooth, centrally concentrated object, exhibiting an elliptical morphology. The color gradient suggests a relatively old stellar population, with a yellowish-orange hue dominating the central region, indicative of evolved stars. There is a slight elongation visible, deviating from a perfectly circular shape. The outer regions appear fainter and more diffuse, fading into the background sky. There is no clear evidence of distinct spiral arms or significant dust lanes. The overall structure suggests a lack of significant recent or ongoing major merger activity, with a generally undisturbed appearance.
