The galaxy presents an overall elliptical morphology, although there are subtle features suggesting a possible disk-like structure. The central region exhibits a significant concentration of light, appearing smooth and relatively featureless with a yellow hue. The galaxy appears moderately elongated with a fairly substantial size. The outer regions are less defined, suggesting a gradual decrease in stellar density with distance from the center. There is some evidence of mild disturbance or interaction, although no clear signs of a major ongoing merger are apparent. The galaxy appears to be actively forming stars at a low rate.
