The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of radial symmetry. The central region displays a concentrated bright core, indicative of a significant stellar population density and potentially a supermassive black hole at its center. The color profile shifts from a warm, reddish hue in the core to cooler, bluer tones in the outer regions, suggesting a transition from older stellar populations in the center to younger, potentially star-forming regions in the periphery. There is little evidence of spiral arms or a well-defined disk structure. Faint irregularities are present which could suggest very minor disturbances but no major merger is observed. The overall appearance suggests a relatively evolved system undergoing limited recent star formation.
