The galaxy presents as a relatively smooth, elliptical-like structure with an apparent disk component. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially an older stellar population, possibly a supermassive black hole. The galaxy appears to be somewhat elongated, more of a disk, but not very much. There are no obvious spiral arm structures visible in this image. The outer regions of the galaxy show a gradual decrease in light intensity, indicating a lower stellar density in the outskirts, with perhaps a halo component that’s fairly symmetrical. The color gradient suggests a shift from bluer star formation regions to older, redder stellar populations towards the core. There are hints of minor disturbances within the galaxy shape and light distribution indicating past interactions. The overall morphology appears relatively undisturbed in this image.
