The galaxy appears to be a relatively smooth, elliptical galaxy. It has a generally round morphology, exhibiting a centrally concentrated, luminous core that gradually decreases in intensity towards the outer edges. There are no discernible spiral arms or significant dust lanes visible. The central region presents a yellowish-white hue, indicative of an older stellar population. A slight elongation is observable, deviating from a perfectly circular shape. There is a subtle suggestion of a minor disturbance in the galaxy's overall structure.
