The galaxy presents as a singular, moderately concentrated light source. The overall morphology appears relatively smooth, exhibiting a profile consistent with an elliptical galaxy. There is a central, bright bulge region that appears roughly spherical in shape. The core of the galaxy exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Fainter, diffuse light extends outwards from the core, with some subtle blueish-green tinges visible in a scattered fashion at the periphery. No distinct spiral arms or bar structures are apparent. There are no obvious signs of ongoing major mergers or significant tidal disturbances in the image.
