The galaxy presents an elliptical morphology, exhibiting a central bulge that appears relatively smooth and centrally concentrated. The light distribution suggests an older stellar population, with a notable lack of prominent blue star-forming regions. There is some irregularity and a hint of a disk or arm-like structure in the outskirts, potentially indicative of a past or ongoing interaction/merger event. The color gradient is subtle, trending from a yellowish core to slightly bluer outer regions, which might suggest a weak gradient in stellar populations. Overall, the galaxy appears to be a relatively massive system with a mix of smooth, evolved components and features hinting at recent or ongoing dynamical processes.
