The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a spheroidal system, potentially an elliptical galaxy or the bulge component of a spiral galaxy seen at a large distance. The galaxy exhibits a yellowish-orange hue, implying an older stellar population and a relatively low rate of on-going star formation. There is no discernible spiral arm structure or significant dust lanes visible within the image. The shape appears largely regular, without major tidal features or signs of recent mergers, though minor disturbances cannot be ruled out at this resolution.
