The galaxy appears to be an elliptical galaxy at a considerable distance, exhibiting a smooth, somewhat spherical morphology. The light profile is centrally concentrated with a gradual decrease in intensity outwards, lacking any distinct spiral arm structures or a prominent disk component. There is a slight elongation present but it appears quite rounded. The color profile suggests a population of older stars with a redder hue, particularly towards the outer regions, indicating limited recent star formation. There is no indication of any major merger events or significant tidal disturbances in the galaxy’s morphology.
