The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, unresolved nucleus. Diffuse light extends outwards from the central region, with a relatively smooth profile, indicating an older stellar population. There is a slight asymmetry in the outer isophotes; however, no strong tidal features or obvious signs of recent major merger events are visible. The galaxy exhibits a slight reddish-yellow hue, consistent with a low star-formation rate. The overall structure suggests an evolved system, likely a massive elliptical galaxy residing at a redshift of approximately 0.16.
