The galaxy presents as a lenticular or possibly an elliptical galaxy, viewed at a significant inclination to our line of sight. It exhibits a centrally concentrated bulge that appears mostly smooth and symmetrical. The bulge displays a color gradient, with a whiter, seemingly higher-intensity core that fades into a yellowish hue towards its periphery. Surrounding the bulge is a disk component, discernible by its flattened shape and slightly bluer color. The disk appears relatively smooth as well, lacking prominent spiral arm structures. The apparent axial ratio suggests a significantly elongated shape. There is no clear evidence of ongoing major mergers or significant tidal disturbances, suggesting that the galaxy is a relatively isolated and evolved system. However, the presence of some irregularities might point to minor interactions in the recent past. Overall, the morphology points towards a galaxy transitioning towards a quiescent state, where star formation is either suppressed or minimal.
