The galaxy presents as a somewhat elongated, lenticular structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a fainter, disk-like component with a greenish tint, potentially indicating the presence of younger stars and ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be slight irregularities or minor disturbances in the outer regions of the disk, but overall, the morphology is relatively smooth. The overall form is moderately elongated.