The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a bright, concentrated luminosity, indicative of a substantial stellar density. The light gradually diminishes from the central region outwards, displaying a diffuse halo. Some subtle, faint blue structures can be seen surrounding the core. These may be a disk, or perhaps sites of more recent star formation, although the resolution makes it difficult to say for sure. There seems to be little to no indication of major disturbances. Overall, the galaxy exhibits characteristics suggestive of a evolved system with ongoing, albeit potentially low-level, star formation.
