The galaxy appears to be elliptical in shape, with a smooth and largely featureless morphology. Its color profile indicates a concentration of older stellar populations, exhibiting a yellowish-red hue particularly towards its center, which suggests a dominant population of evolved stars and potentially a higher metallicity in the core. The outskirts exhibit slightly bluer colors suggesting a small amount of younger stars. The galaxy is relatively concentrated, showing a high degree of central luminosity. There is no apparent disk structure or spiral arm formation. No signs of major mergers or tidal disturbances are observed. The overall structure suggests a galaxy undergoing minimal current star formation activity, although some ongoing activity is present.
