The galaxy presents as an edge-on spiral, or possibly a lenticular, system. A prominent central bulge is visible, appearing somewhat elongated and rounded. There is some evidence of a disk structure, thin and extending outward from the bulge. The disk material appears smoother and less resolved than the bulge. There may be the presence of some dust lanes attenuating the light from the disk, but this is difficult to confirm at the image resolution. The overall color profile suggests an older stellar population, with the bulge exhibiting a yellower hue than the fainter blueish disk. There are no signs of significant morphological disturbances or ongoing major mergers.
