The galaxy presents as a largely smooth, elliptical-like object with a concentrated central bulge that exhibits a yellow-white hue, indicating an older stellar population. The overall shape is fairly round. There is a faint disk structure, although subtle, showing minor features, and little evidence of spiral arms. The galaxy's periphery fades gradually into the background sky, suggesting a diffuse outer halo. There is no apparent major disturbance to the overall structure, thus likely an isolated system.
