This galaxy presents as a flattened, disk-like structure seen nearly edge-on. A prominent central bulge is observed, exhibiting a yellowish-orange hue, suggesting an older stellar population likely composed of Population II stars. The disk appears to be relatively smooth with faint hints of dust lanes, primarily along the galactic plane. The lack of distinct spiral arm structures indicates a system potentially lacking recent major star formation events. The galaxy appears relatively undisturbed, without significant morphological distortions suggestive of ongoing or recent major mergers. The overall light distribution suggests a centrally concentrated system with luminosity decreasing outwards from the bulge into the fainter disk.
