The galaxy presents an overall elliptical morphology, appearing somewhat smooth and concentrated. The central region exhibits a yellowish-orange hue, potentially indicating an older stellar population dominated by redder stars, and/or dust obscuration. There may be a possible slight asymmetry or minor disturbance present in the structure, although the image resolution makes this difficult to ascertain conclusively. The galaxy shows little evidence of ongoing major star formation. The estimated physical size indicates that this is a large and massive galaxy. 
