The galaxy appears as a relatively smooth, elliptical structure with a pronounced central bulge. There's a hint of a disk-like structure, though it's not strongly defined. The light distribution suggests a centrally concentrated stellar population. Color gradients are subtle but present, transitioning from a more reddish-orange hue in the core to a slightly bluer tint in the outer regions, suggestive of differing stellar populations. There is a minor asymmetry or distortion in the outer regions, potentially hinting at past or ongoing interactions, though no major merging events are apparent. The galaxy exhibits a modest degree of elongation, deviating somewhat from a perfectly circular shape.
