The galaxy presents as a highly elongated object, indicative of a disk galaxy viewed at a significant inclination. The central region exhibits a noticeable concentration of light, suggesting a bulge or a more densely populated stellar core. Faint, diffuse extensions are visible along the major axis, typical of spiral arms or tidal features. The color gradient across the galaxy appears relatively smooth. There is subtle hint of dust lanes or obscured regions in the disk plane, contributing to the galaxy's overall structure. The galaxy shows no obvious signs of significant ongoing merger activity. 
