The observed galaxy presents as a disk-like structure viewed at a high inclination, close to edge-on. The central bulge appears prominent and exhibits a yellowish-orange hue, potentially indicative of an older stellar population. The disk component displays a more diffuse and elongated morphology, fading in intensity towards the outer edges. There appears to be a bright knot of light within the disk on one side of the bulge. The overall shape and light distribution suggest possible disturbances or interactions. The disk's structure implies possible warping or asymmetry. The central bulge and disk contrast in color; the bulge's yellower hue indicates evolved stars, whereas the disk shows signs of ongoing or recent star formation, but the signs are minimal.
