This galaxy appears to be a late-type spiral galaxy, seen almost edge-on. A prominent central bulge is visible, exhibiting a smooth, rounded morphology. The disk of the galaxy appears relatively thin and elongated, with evidence of dust lanes along the galactic plane. Based on the color distribution, the bulge appears to contain an older stellar population with a yellow-orange hue. The disk exhibits bluer regions, indicative of more recent star formation. No significant tidal distortions or signs of major mergers are detected. Minor disturbances of the morphology may be present, but this should be verified with a higher resolution image.
