The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall color appears to be slightly reddish, indicative of an older stellar population. The galaxy's form is mostly round. There is only very weak evidence of any significant disturbance to its shape. The color gradient suggests a gradual fading of light intensity from the core outwards. There are no obvious signs of active star formation regions such as bright knots or spiral arms.
