The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity outward from the core. The galaxy has a generally round morphology with some suggestion of deviation toward a slight cigar shape. There is no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy shows no major signs of ongoing merger activity or significant tidal disturbance. The light appears largely homogenous across the body.