The galaxy presents as a fairly smooth and rounded elliptical system. Color gradients across the body are subtle. The core appears slightly brighter than the outer regions. It appears relatively undisturbed with no clear evidence of a major ongoing merger or strong tidal interactions, however, there is a possibility of a very slight disturbance. Its integrated light suggests a galaxy with intermediate mass for its type and with a very low rate of star formation. It shows low intensity in blue wavelengths. Most likely it is composed of older stellar populations.