The galaxy presents a largely smooth and elliptical morphology. It exhibits a dominant central bulge, which is bright yellow-orange, indicating an older stellar population with lower levels of current star formation. There appears to be little evidence of spiral arm structure or dust lanes within the galaxy. The galaxy's shape is mostly round. Faint, blueish diffused light surrounding the galaxy can be seen. No major signs of galactic merging or major disturbances are observed.