The galaxy presents as a luminous, relatively compact object with a smooth, elliptical morphology. It exhibits a yellow-orange hue, suggesting a stellar population that is evolved and dominated by older stars. The high degree of roundness and lack of discernible disk-like features indicate a classification leaning towards an elliptical galaxy type. There are no signs of significant ongoing mergers or major disturbances in the galaxy's structure, the galaxy appears to be a relaxed, quiescent system.
