This galaxy presents a largely smooth morphology. The light is concentrated towards the center, which exhibits a distinct yellowish hue, potentially indicating an older stellar population. A gradual falloff in light intensity is observed radially outward from the core. The galaxy appears to be mostly spheroidal. There are hints of subtle disturbances, potentially indicating a minor interaction with another galaxy, or recent minor merger event. However, there is no clear disruption to the primary structure and it still appears mostly smooth. This galaxy is relatively massive, and has likely shut down its star formation within its interior regions. 
