The galaxy appears to be a spiral galaxy, exhibiting well-defined spiral arms. The arms are tightly wound around a bright central bulge. The bulge appears to be moderate in size, neither dominating nor insignificant compared to the overall disk. Faint hints of a bar structure may be present, but it is not prominently featured. Two dominant spiral arms are visible. No clear signs of major galactic mergers are apparent, though subtle disturbances cannot be ruled out. The disk component is viewed at an angle that is nearly face-on, with minimal apparent inclination. The color distribution indicates a relatively uniform population, with possible variations in the spiral arms suggesting areas of differing stellar populations or dust obscuration.
