The galaxy presents as a slightly elongated, lenticular system, exhibiting a moderate degree of ellipticity. It has a notable bulge component, with a smooth, centrally concentrated light distribution, which comprises the brighter, yellowish core of the galaxy. Surrounding the central bulge, there's evidence of a fainter, more diffuse disk. It has a bluer overall color, suggesting active or recent star formation. The isophotes appear relatively regular, lacking strong signs of tidal disturbances or major mergers. The galaxy presents a system that is in the transition between spiral and elliptical morphology.