The galaxy presents as a centrally concentrated elliptical type, exhibiting a smooth morphology with a high degree of symmetry. Its shape is somewhat elongated, deviating slightly from perfectly circular. The color profile suggests an older stellar population, dominated by yellow and red hues, characteristic of stars nearing the end of their life cycle. There is minimal evidence of distinct spiral arms or active star formation regions. The overall appearance indicates a relatively quiescent galaxy, likely having exhausted much of its gas and dust. No signs of tidal disturbances or ongoing mergers are apparent. 
