The galaxy presents as a flattened, disk-like system, viewed at a shallow angle relative to its plane. It exhibits a prominent, centrally concentrated bulge, appearing roughly spheroidal and possessing a yellowish-orange hue, suggestive of an older stellar population. The disk component is subtly visible and possesses a bluer color, indicating the presence of younger stars and active star formation. There is no prominent bar feature visible. No distinct spiral arms are detected, however, subtle deviations in the disk's structure hint that spiral arms may be present, albeit weakly defined or tightly wound. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers.
