The galaxy presents as a generally smooth, centrally concentrated light distribution. It exhibits a roughly rounded morphology. There is a subtle suggestion of possible minor disturbances or tidal features, but the overall structure appears relatively undisturbed. The galaxy's color profile indicates it is more luminous in the green wavelengths than in the red or blue. The overall appearance suggests an elliptical or lenticular galaxy type. There is potential for this to be a merging event, but there are not obvious indications of violent interactions. 
