The galaxy presents as a lenticular or early-type spiral galaxy. It is characterized by a smooth, elliptical light distribution, concentrated towards the center with a prominent bulge. The galactic disk is observed nearly edge-on, indicated by its elongated shape. There's a noticeable color gradient, transitioning from a yellowish-white core to a slightly bluer hue towards the outer edges, potentially indicating older stellar populations in the central region and younger stars in the disk. No distinct spiral arm structures or dust lanes are visible. The galaxy does not appear to be undergoing any major mergers or tidal disturbances. The morphology suggests a galaxy that has largely completed its star formation.
