The galaxy appears to be a luminous, elliptical system. Its core exhibits a bright, concentrated luminosity, surrounded by a more diffuse halo. The galaxy exhibits a smooth, symmetrical morphology with no apparent spiral arm structures. The color profile suggests a higher concentration of older stellar populations, particularly towards the center, emitting more light in the redder wavelengths. There are no apparent signs of active star formation, major mergers, or tidal disturbances. Based on its morphology, it likely represents an evolved, relatively quiescent galaxy with a substantial stellar mass.
