This galaxy presents as an elongated, lenticular shape, exhibiting a smooth and relatively featureless morphology. Its orientation is close to edge-on from our perspective. The central bulge appears to be a yellowish-orange hue, suggesting an older stellar population. Fainter extensions are visible on either side of the bulge, likely representing the galactic disk. These extensions have a slightly bluer color compared to the bulge, which could indicate the presence of younger, hotter stars, though not in significant quantities. No distinct spiral arm structures or dust lanes are discernible within the disk, furthering the notion of an evolved system. The overall symmetry of the galaxy suggests it is relatively undisturbed, with no significant signs of ongoing mergers or interactions.
