The galaxy presents a distinct, elongated morphology, appearing nearly edge-on with a high degree of inclination relative to our line of sight. The central region exhibits a significantly higher luminosity, gradually decreasing towards the outer edges. The galactic nucleus is not clearly resolved. There is a clear color gradient observed, ranging from blueish tones at the poles to a redder hue on the galactic plane. There is little evidence of spiral arm structure due to the edge-on orientation. The overall form is fairly smooth and without strong signs of recent merger activity or tidal disturbances. Based on its red color and smooth structure, I suspect it may be a late-type spiral galaxy. 