The galaxy appears to be a relatively smooth elliptical galaxy. It exhibits a high degree of central concentration with a bright, compact core that fades smoothly outward. There is very little evidence of spiral arm structure, star forming regions, or dust lanes. The ellipticity of the galaxy is moderate, displaying a somewhat flattened appearance. The overall color is slightly redder, suggesting an older stellar population, with little ongoing star formation. The galaxy shows no signs of major disturbances or mergers.
