This galaxy appears to be a relatively smooth, elliptical system. Its core is a bright, concentrated yellow-white, suggesting an older stellar population dominates the central region. Moving outward from the core, the galaxy transitions to a faint bluish halo. This halo implies the presence of a younger, bluer stellar population than in the core, and a small amount of ongoing star formation is likely occurring. The overall round morphology suggests a classification as an elliptical galaxy, and there is no obvious indication of spiral arms or a prominent disk structure. There is no visual evidence of any major mergers or significant tidal disturbances in the image, suggesting it is a relatively relaxed and settled system.
