The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. It exhibits a golden hue, with a very slight color gradient that indicates subtle color changes. The galaxy appears generally undisturbed, with no significant tidal features, asymmetries, or signs of recent major merger activity. No distinct disk component is visible. The structure is characterized by a high degree of central concentration. Based on this, the galaxy is likely a relatively massive system, that is undergoing a low rate of star formation. 
