This galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright and somewhat yellowish-white, suggesting an older stellar population likely dominated by evolved stars. A more diffuse, bluish halo surrounds the core, possibly indicating the presence of a younger stellar population or ongoing, though limited, star formation in the outer regions. The galaxy is elongated, with a moderate ellipticity, though overall quite round. There is no obvious indication of strong tidal interactions or major mergers, but a possible subtle distortion hints at a minor disturbance or interaction in its past. Overall, the galaxy appears to be a relatively massive system, with ongoing low levels of star formation.
