The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge that is luminous in the observed wavelengths. The isophotes gradually fade as one moves radially outward from the core, suggesting a diffuse halo. There are hints of a very faint, flattened disk, but the object presents primarily as a spheroid. The overall morphology suggests an evolved system, possibly a lenticular galaxy approaching the end-stage of galaxy evolution. Evidence of current major merger activity is not obvious based on the image.
