The galaxy appears as a relatively smooth, elliptical-shaped object with a concentrated central bulge. The light distribution suggests a gradual decrease in brightness from the core outwards, consistent with an elliptical morphology. There is little evidence of spiral arms or other distinct features typically associated with disk galaxies. The galaxy exhibits a color gradient, transitioning from a yellowish core to a slightly bluer halo. Overall, the galaxy shows no signs of major disturbances or ongoing mergers, but minor asymmetrical features are potentially present.
