This galaxy presents a complex structure, appearing as a spiral galaxy viewed at an oblique angle. The central bulge is prominent and displays a smooth, concentrated distribution of light, suggesting an older stellar population. Fainter spiral arms emanate from the central region. These arms are tightly wound, hinting at a more evolved spiral morphology. The disk component seems relatively thin, and its orientation contributes to the elongated appearance of the galaxy. Within the spiral arms, subtle variations in color and brightness are observed, indicating regions of active star formation intermixed with areas of older stellar populations and dust lanes. The galaxy exhibits a notable inclination with respect to the observer, leading to a foreshortened view of its overall disk structure.
