The galaxy appears to be a relatively smooth, centrally concentrated system. It presents a noticeable, though somewhat diffused, halo extending outwards from the core. The central region exhibits a bright, luminous core, suggesting a significant concentration of stars or an active galactic nucleus. Faint, extended features may indicate a disk structure, but the overall morphology is somewhat blurred. The color distribution appears slightly redder in the central region, possibly indicating an older stellar population, while the outer regions show hints of bluer colors, potentially indicative of ongoing star formation, albeit at a low rate. There may be some minor disturbances in the overall shape, but no major merger events are visibly apparent. Overall, it looks like a large elliptical galaxy with some disk features, with minimal signs of strong star formation, but possible subtle ongoing star formation.
