The galaxy presents as a somewhat elliptical, relatively smooth structure. It appears as a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy displays a yellowish-orange hue, suggesting an older stellar population, with a low star-formation rate and a high mass, indicating it may be a fully developed galaxy. There are no spiral arms immediately visible, and the lack of intense blue light further indicates an absence of significant recent star formation within the galaxy. The outer edges of the galaxy are not sharply defined, suggesting a gradual transition into the surrounding space. The shape of the galaxy is not perfectly circular, but is rather elongated. Overall, it appears to be an evolved galaxy with a well-defined structure, likely at a considerable distance, indicated by its small angular size. There are no distinct tidal tails or asymmetries to suggest any recent major merger events, but there is some evidence of minor disturbances.
