The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy is generally round, with a slight deviation from perfect circularity. There is no apparent dust lane or spiral arm structure visible in this image. The color profile suggests a population of older stars, indicated by the reddish-yellow hue, with a minimal presence of young, blue stars. There are no signs of any major disturbances or ongoing mergers. The overall structure suggests a well-established, mature galaxy with minimal recent star formation activity.
