The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, with a noticeable fall-off in luminosity towards the outer regions. The light distribution suggests an older stellar population, with a color profile that is more red in the inner regions and outer regions. There is no clear evidence of spiral arms or dust lanes. The overall morphology indicates that it is likely an early-type galaxy. There are some minor asymmetries, but it is likely undisturbed.
