The galaxy presents as a fairly smooth, centrally concentrated object. It appears to be elliptical in shape, with a slight elongation. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population and/or significant dust obscuration. There is a subtle color gradient extending outward from the core, transitioning to a redder, less intense light in the outer regions. No distinct spiral arms or features are visible. The overall appearance suggests a relatively evolved system with no signs of ongoing major mergers or significant star formation. The light distribution is smooth and gradually tapers off towards the edges of the galaxy.
