This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The overall shape appears to be elliptical, but there are slight deviations. The galaxy displays a gradient in color, transitioning from a yellowish-white core to bluish outer regions. There is no obvious spiral structure or distinct dust lanes, and no signs of recent or major merger activity. It shows a somewhat high likelihood of being an elliptical galaxy. The low level of detected star formation suggests that it is populated by an older stellar population.
