The galaxy presents as a somewhat elongated, lenticular-like structure. It exhibits a smooth, centrally concentrated bulge that transitions gradually into a fainter, more diffuse disk. The color profile suggests an older stellar population, with a yellowish hue dominating the central bulge and extending into the inner regions of the disk. There is a subtle indication of bluer colors in the outer regions of the disk, suggestive of recent or ongoing star formation, albeit at a low rate. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers. The overall morphology suggests a relatively evolved system with a substantial mass.
