This galaxy presents as a centrally concentrated object, exhibiting an elliptical morphology. The core region displays a bright, intense luminosity. Moving outward from the core, the luminosity gradually decreases, suggesting a smooth distribution of stellar populations. There is evidence of a faint disk-like structure surrounding the central bulge, although its features are somewhat diffused. This disk may be exhibiting signs of disturbances, with some areas appearing more irregular than others. There appears to be some evidence of a potential ongoing merger, with a significant disturbance on the left side. Overall, this galaxy shows characteristics indicative of a massive, evolved system, with potential ongoing interactions influencing its morphology.
