The galaxy presents as a smooth, elliptical-like structure, displaying a concentrated central bulge. The light distribution is not uniform; it appears brightest towards the core and gradually fades outwards. The color gradient suggests an older stellar population, exhibiting a yellowish-red hue. There may be a slight indication of a disk, but that is very slight. Based on its morphology it appears to be in a relatively settled state, showing no visible signs of any major merger events.
