This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. The light distribution is concentrated towards the center, indicating a higher density of stars within the galactic nucleus. There is a gradual decrease in luminosity outward from the core, forming a diffuse halo. The galaxy appears quite round in shape. There is no prominent disk-like structure, nor is there evidence of any ongoing major mergers or significant tidal disturbances. Minor distortions could exist, but the resolution does not permit this to be confirmed. The color suggests that the stellar population consists mainly of older stars. It's likely a very massive system with relatively low current star formation.
