The galaxy appears as a somewhat elliptical structure with a smooth, concentrated central bulge. The color gradient suggests a population of older stars, with a redder hue dominating the core. There's a subtle transition to a slightly bluer, less distinct outer region, implying some ongoing, albeit subdued, star formation. No clear spiral arm structures or prominent dust lanes are discernible. Overall, the morphology points towards an early-type galaxy, possibly an elliptical or lenticular galaxy transitioning to a red and dead state. There are no visible signs of a major merger, but minor disturbances cannot be ruled out at this resolution.
