The galaxy presents an elongated morphology, indicative of a disk galaxy viewed at an angle. The central bulge is moderately prominent, appearing with a yellowish-white hue. Surrounding the bulge is a disk structure. Spiral arms are visible, although somewhat tightly wound, and extend outwards from the central region. The spiral arms exhibit a bluer color, suggesting regions of active star formation. The dust lanes are subtly visible within the spiral arms, providing a sense of depth. The galaxy appears relatively isolated with no clear signs of major interaction or ongoing merger events. Overall, the galaxy appears to be a well-defined, disk-dominated system with clear spiral structure.
