The galaxy presents as a centrally concentrated, relatively smooth system. Its morphology is largely elliptical, showing high central luminosity that gradually decreases with radial distance. The color profile suggests an older stellar population, exhibiting a redder hue towards the core and gradually bluer as you move further from it. There's little evidence of spiral arm structures or significant dust lanes. The overall appearance indicates a galaxy with a high degree of symmetry and structural coherence, lacking any clear signs of major disturbances or ongoing mergers.
