The observed galaxy appears as a centrally concentrated, relatively smooth elliptical galaxy. Its light profile exhibits a high degree of symmetry, with a gradual decrease in intensity from the core outward. The dominant color is yellow, suggesting a population of older stars. There is no observable dust lane or spiral arm structure, indicating a lack of significant ongoing star formation. The overall morphology indicates a mature system, likely with a significant stellar mass. The galaxy is roughly circular in appearance, showing minimal elongation, which could indicate that it has nearly spherical symmetry. There are no visible signs of any recent or ongoing merger events.
