The galaxy presents as a centrally concentrated, luminous object with a smooth, elliptical morphology. Its overall color is a warm, yellow-orange, suggesting a stellar population dominated by older, redder stars. There's a gradual decrease in luminosity moving from the core outwards, indicating a fairly uniform distribution of stellar density, consistent with an early-type galaxy. There are no visually discernible spiral arms or dust lanes, and the smoothness of the light distribution doesn't suggest any ongoing major merger activity or significant tidal disturbances. The galaxy appears slightly elongated, but not to a degree indicating a highly flattened disk. The lack of distinct blue regions or HII regions indicates a relatively low rate of recent star formation.
