The galaxy presents as an elliptical morphology, appearing largely smooth and possessing a concentrated central bulge. It exhibits a yellowish hue, indicating a population of older stars and a dearth of ongoing, significant star formation. There may be a faint disk structure. The galaxy is moderately bright, but relatively small in apparent size on the sky. There is no obvious indication of active galactic nuclei or significant dust lanes. No merging is taking place with other objects.
