The galaxy presents a distinctly edge-on morphology. A prominent central bulge is visible, exhibiting a smooth and concentrated distribution of light. The bulge appears to be slightly elongated. A disk component surrounds the bulge, also viewed edge-on. The dust lane appears thin or is not easily resolvable with this resolution. The overall color of the galaxy shows a reddish to yellowish-orange hue, particularly towards the central bulge. This coloration suggests an older stellar population dominating the light emission, possibly indicative of reduced star formation activity. The galaxy appears to be relatively isolated with no obvious signs of major interaction with neighboring galaxies. The outskirts appear faint.
