The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, indicative of a large bulge component. The color is predominantly yellowish-red, suggesting an older stellar population and relatively low ongoing star formation. There is a faint, diffuse halo surrounding the central region. There are no obvious spiral arm structures or dust lanes visible. There is a possibility of a minor disturbance in the outer reaches of the halo region. The galaxy appears relatively undisturbed, with no major signs of mergers or tidal interactions.
