The galaxy appears to be a relatively smooth, elliptical galaxy. The light is concentrated towards the center of the galaxy, which exhibits a yellowish hue, possibly indicating an older stellar population dominating the core. The outer regions display a bluer color, which could mean they are indicative of more recent star formation and a younger stellar population, although there are few distinct features and a smooth gradient in the image between the core and the outskirts. There's no strong evidence of a spiral arm structure or significant dust lanes from the image, lending support to the suggestion that it is an elliptical galaxy with a relatively passive star formation rate.
