The galaxy presents a largely smooth, elliptical morphology with a high degree of roundness. Its color profile indicates a redder population of stars, suggesting an older stellar population and a relatively low rate of on-going star formation. There is no discernible disk structure and lacks prominent spiral arms. There are no obvious signs of major tidal disturbances or a recent merger event. Any merging that may be occurring appears to be minor, or a past merger. The galaxy is a bright elliptical galaxy. 
