The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The intensity of light diminishes gradually towards the outer regions, which are composed of fainter, reddish hues. The lack of apparent spiral arm structures or significant dust lanes indicates that this galaxy is most likely an elliptical or lenticular type galaxy. The overall shape is slightly elongated, but not excessively so. There are no signs of any major ongoing merger events or tidal disturbances.