This galaxy exhibits a moderate redshift, suggesting a significant distance. Morphologically, it appears largely smooth, with a possible hint of a disk-like structure or a faint feature. The galaxy is elliptical, though it is elongated along one axis. The color gradients suggest variation in stellar populations, or perhaps dust obscuration. It may be undergoing a minor interaction, as evidenced by some slight distortions, or simply be a galaxy with internal substructure that suggests a recent merger event.
