The galaxy presents as a relatively smooth, centralized structure with a noticeable concentration of light towards the core. The galaxy exhibits a subtle, almost imperceptible disk-like structure. The overall color gradient transitions from a yellowish core to a bluer outer halo. The light distribution suggests that the galaxy is not experiencing major disturbances, with only minor asymmetries. The morphological analysis suggests this is likely an elliptical galaxy with a high fraction of old stars but there is possibly ongoing, albeit slow, star formation within the galaxy. The galaxy exhibits a redshift, indicating its considerable distance from us. 
