The galaxy presents as an elliptical morphology, displaying a smooth, diffuse light profile. The color appears to be a yellowish-white, indicating an older stellar population. There is a slight elongation, though the aspect ratio is close to unity, which suggests that it is close to circular. No distinct spiral arms or prominent dust lanes are discernible. The central region exhibits a higher concentration of light, suggestive of a galactic bulge. Overall, the morphology aligns with that of a relatively massive galaxy with a considerable formation history.
