The galaxy presents a generally elliptical morphology with a smooth, centrally concentrated light distribution. The core exhibits a high surface brightness, gradually decreasing towards the outer regions. A faint, extended halo is suspected, but the signal-to-noise ratio makes it difficult to discern definitive structural features at the limits of the galaxy. The overall color appears relatively uniform across the galaxy, with a subtle reddening towards the center. No prominent spiral arm structures or dust lanes are apparent. The lack of discernible substructure suggests a relatively evolved system, potentially an early-type galaxy.
