The galaxy appears to be an elliptical morphology. It exhibits a relatively smooth light distribution, lacking distinct spiral arms or a prominent central bar. The primary body of the galaxy is substantially round. The galaxy displays a color gradient, transitioning from a reddish hue at its core to a more greenish or yellow-green periphery. This suggests a potentially older stellar population concentrated towards the center, and some amount of on-going star formation further away. There is no obvious signs of tidal disruption or ongoing merger activity. 
