The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is approximately round, with no obvious signs of a disk-like structure or spiral arms. There is a subtle color gradient visible, with the central region exhibiting a slightly redder hue compared to the bluer outer regions. This color difference suggests a potential variation in stellar populations or dust content between the core and the periphery. There is a slight irregularity in the shape, hinting at a possible minor disturbance or interaction, although it is subtle. The galaxy exhibits a low level of ongoing star formation. Overall, the galaxy is a large elliptical galaxy.
