The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. Its color profile suggests a dominant population of older stars, with a yellowish-orange hue indicative of lower star formation activity. The galaxy appears somewhat elongated, with no prominent spiral arm structures or dust lanes visible. There is no distinct nucleus visible, and there are no indications of significant tidal disturbances or ongoing merger activity. The light is centrally concentrated, indicating an elliptical morphology, viewed at an angle. Based on its apparent color and form, it appears to be a passively evolving system.
