The galaxy appears as a singular, centrally concentrated object. The morphology suggests an elliptical type, dominated by a smooth, spheroidal structure with no discernible spiral arms or disk-like features. The light profile is smooth and relatively uniform.

The color index suggests a composition of older stellar populations, indicating a relatively passive star-forming history. There is no visible evidence of ongoing major mergers or tidal disturbances, suggesting that the galaxy is relatively isolated. The high level of smoothness further supports the classification of an elliptical galaxy, characterized by its well-mixed stellar populations.
