The observed galaxy exhibits an elongated morphology, consistent with an edge-on disk galaxy. A prominent central bulge is visible, displaying a smooth, concentrated luminosity profile. The disk component appears relatively thin and extended, with subtle color variations suggesting potential dust lanes or regions of differing stellar populations within the disk. The galaxy shows no apparent signs of major tidal distortions or ongoing mergers based on visual inspection. The bulge is relatively large compared to the disk. The galaxy exhibits a red-shifted spectrum, characteristic of galaxies at considerable distances.
