The galaxy presents as a relatively smooth, centralized object with a round morphology. Color gradients indicate some variation in stellar populations across the galaxy. A central concentration of yellow light suggests a bulge with an older stellar population. The overall structure indicates the galaxy is likely an elliptical. There is no definitive evidence of spiral arm structure or a significant disk component visible. The galaxy does not display signs of major disturbances or ongoing merging activity, though some minor asymmetry might be present. The color indices imply a moderate redshift. Based on these observations, the galaxy appears to be a massive system.
