This galaxy appears to be a relatively smooth, round object, potentially an elliptical galaxy or a lenticular galaxy seen face-on. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population and possibly an active galactic nucleus. The galaxy displays a color gradient, shifting from a bluer hue at the center to a redder tinge in the outer regions. This suggests a variation in stellar populations, with younger, hotter stars dominating the core and older, cooler stars residing in the outskirts. There is minimal evidence of spiral arm structure or significant dust lanes. Overall, the morphology suggests a galaxy that has undergone significant evolution, with a relatively quiescent star formation history.
