The galaxy appears as a diffuse, elliptical object. It exhibits a smooth morphology with a high degree of central concentration. The core is a bright yellowish-white, suggesting an older stellar population. Moving outward from the core, there's a gradual transition to a fainter greenish halo, possibly indicating ongoing or recent star formation in the outer regions. The galaxy has a moderate ellipticity, appearing more elongated than perfectly circular. No distinct spiral arms or bars are discernible within the observed structure. There's no obvious evidence of strong tidal interactions or major mergers, although subtle asymmetries may suggest minor disturbances. The overall color profile indicates a evolved system with residual star formation.
