The galaxy presents a flattened, elongated morphology, suggestive of a disk-like structure viewed at a steep angle. The central region exhibits a concentrated, bright bulge, appearing yellowish-orange in color, which likely indicates an older stellar population. The disk component appears relatively smooth with a bluer hue, fading in intensity with increasing radial distance from the galactic center. No distinct spiral arm structures or prominent dust lanes are readily apparent in the visible spectrum. There are no major disturbances or interactions evident in the image, although there may be minor disturbances in the disk. The overall shape is reminiscent of a lenticular galaxy.
