The galaxy presents a roughly circular morphology, appearing largely smooth with a concentrated central bulge region. This core is a bright, intensely luminous source. Surrounding the core is a less defined region. The color profile exhibits a noticeable shift from a bluer hue in the central core to a greenish-blue in the outer regions of the galaxy. This shift may indicate differing stellar populations or dust extinction gradients. Evidence of a disk is not apparent. The morphology appears relatively undisturbed with only a few minor distortions, suggesting it is not currently undergoing a major merger event.
