The galaxy appears to be a relatively small, elliptical galaxy. Its morphology suggests it is fairly smooth, with a high degree of central concentration. The roundness indicates it is closer to an E0 type galaxy. There are no clear spiral arm structures or significant dust lanes visible, implying a lack of ongoing, major star formation. It exhibits a faint blueish hue, suggesting a possible, small population of young stars. The low star formation rate also indicates the galaxy is likely a red and dead galaxy with little ongoing stellar genesis. There is no clear evidence of tidal disturbances or ongoing merger activity, which is further supported by the lack of morphological asymmetry. Overall, the galaxy appears to be a quiescent elliptical galaxy.
