The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated morphology. There is little evidence of spiral arms or disk-like structure. The galaxy's light profile is relatively round, without significant elongation. The color gradient suggests an older stellar population throughout the galaxy, particularly in the central region, implying a lack of recent star formation. No obvious signs of tidal disturbances or ongoing mergers are apparent, though there is a hint of minor asymmetry. The overall structure suggests a system that is relatively relaxed and evolved.
