The galaxy appears as a centrally concentrated object with a smooth morphology. The light profile suggests an elliptical or lenticular type galaxy. The primary body of the galaxy exhibits a relatively uniform color, with a slight redder hue compared to the bluer objects in the surrounding field. This reddening may indicate an older stellar population. There is a subtle extension of light along one axis, hinting at a possible disk-like component. Overall, the galaxy exhibits minimal signs of ongoing star formation or significant dust lanes. There are also no obvious signs of tidal features or major disturbances, suggesting a relatively relaxed system.
