The galaxy presents a generally smooth morphology, appearing largely undisturbed. It exhibits an elliptical shape, with a slightly elongated structure. The light is relatively uniform, indicating a lack of strong spiral arms or distinct features. A color gradient is observed, where the central region of the galaxy appears more reddish, while the outer regions are bluer. This color difference suggests varying stellar populations and ages within the galaxy. The redder core might indicate an older population of stars, while the bluer outer regions may signify younger stars. Overall, the galaxy gives the impression of a mature galaxy, with a somewhat passive star formation history.
