The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. The core exhibits a bright, yellowish-white glow, suggesting an older stellar population. The light gradually fades toward the outer regions, which appear slightly more reddish. There's no indication of significant spiral arm structures or prominent dust lanes. The galaxy appears to be relatively undisturbed, with no major signs of mergers or tidal interactions, although there may be a very minor disturbance in the outer disk. The overall morphology points to a galaxy that is likely nearing the end of its star formation period.
