The galaxy presents as a relatively smooth object with an overall elliptical morphology. It exhibits a concentrated central bulge that appears yellowish. The outer regions of the galaxy gradually fade into the background sky, suggesting a lack of distinct spiral arms or complex structures. There might be some minor disturbance due to the slightly uneven and blurry appearance of the outer edges of the galaxy. The color gradient across the galaxy indicates that the central bulge is composed of older stars. There is no indication of active star formation within the disk.
