The galaxy presents as an edge-on spiral, with a prominent central bulge. The bulge exhibits a yellowish hue, possibly indicating an older stellar population and lower levels of current star formation. The disk component is visible as a flattened structure extending from the central bulge, also possessing a yellowish colour. There's no obvious dust lane, but that doesn't mean it's not there, it could be faint. There is no evidence of major tidal disturbances or ongoing mergers based on the image. It does appear largely undisturbed.
