The galaxy presents as a centrally concentrated system with a smooth light distribution. It exhibits a notable radial color gradient, transitioning from a yellowish-white core to redder, fainter outer regions. There are no clear spiral arm structures or dust lanes visible, suggesting a relatively evolved morphology. The galaxy's shape appears slightly elongated, deviating minimally from a perfect circle. No major ongoing merger events or significant tidal disturbances are immediately apparent, though subtle irregularities might be present upon closer examination. The overall appearance is consistent with that of an elliptical galaxy.
