The galaxy presents an approximately elliptical morphology. The central region exhibits a high surface brightness, appearing nearly unresolved and white in color, suggestive of a significant concentration of stars. The surrounding halo is more diffuse, showing a gradual decrease in intensity outwards. The halo displays a bluish tint, potentially indicating the presence of a younger stellar population or ongoing star formation within the galaxy. No obvious spiral arm structures or bar features are discernible. The galaxy appears relatively smooth in its overall structure, showing only minor asymmetry. There is no clear evidence of any major tidal disturbances or ongoing merger activity.
