The object appears to be an elliptical galaxy at a redshift of approximately 0.1745. The galaxy presents a largely smooth morphology, lacking any prominent spiral arms or distinct features typically associated with ongoing star formation. The light distribution is concentrated towards the center, suggesting a prominent bulge component, with a gradual decrease in surface brightness towards the outer regions. There is very little disk visible, and what might be disk, is very smooth. The general color indices suggest a relatively old stellar population, indicative of minimal recent star formation activity and is relatively massive, consistent with its classification. The galaxy does not show signs of recent major merger events or significant tidal disturbances.
