The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. A disk component is potentially present, but subtle. The color appears moderately red, implying an older stellar population, although some bluer components are visible. The galaxy displays no strong signs of tidal disturbances or ongoing major mergers, and appears relatively undisturbed. The isophotes are elongated but reasonably regular, with a slight ellipticity. There is no significant dust lane apparent. The surface brightness profile appears centrally concentrated, lacking pronounced spiral arm structures.