The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. The light profile suggests a high degree of central concentration, indicated by the bright, yellowish core. There is a gradual decrease in surface brightness moving outward from the center, with the outer regions exhibiting a bluer hue compared to the core. This suggests ongoing, but low-level, star formation in the outer regions, or a population of younger, bluer stars. There is no evidence of spiral arms or a distinct disk structure, implying a dynamically relaxed system. The overall shape is generally round, with no obvious signs of tidal interactions or major disturbances. It is likely to be a mature galaxy that has undergone significant evolution.
