This galaxy appears to be a spiral galaxy viewed nearly edge-on. It displays a flattened disk structure with a prominent central bulge. The bulge exhibits a yellowish-white color, suggesting an older stellar population. The disk shows evidence of dust lanes and a slight blue tint, possibly indicating the presence of younger, hotter stars and ongoing star formation within the spiral arms, though these features are somewhat muted. There's no obvious sign of interactions or major disturbances; however, some subtle asymmetry in the disk hints at possible minor gravitational disturbances. The overall morphology points towards a well-defined disk galaxy with a developed bulge.
