The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. The light distribution appears centrally concentrated, fading gradually towards the outer edges. The galaxy exhibits a subtle elongation, with the major axis oriented vertically in the image. Color gradients are subtle, with a hint of yellow in the core region, suggestive of an older stellar population. Fainter, bluer light is observed in the outer regions, potentially indicative of more recent star formation, albeit at a low level. There is no obvious evidence of spiral arms or a well-defined disk. The overall morphology suggests a system that has largely completed its major merging activity, although minor disturbances cannot be ruled out based on this image alone.
