The galaxy presents a clear disk-like morphology, though not perfectly edge-on. There is a noticeable central bulge, which appears moderately sized in relation to the overall galactic structure. While the bulge appears to be smoothly distributed, there are faint, yet distinguishable, spiral arm structures. The arms are somewhat patchy and not as well-defined, but appear to be separated and emanate from the central bulge. The color of the spiral arms appears more blue compared to the bulge region, suggesting active star formation in these areas. There is no obvious central bar feature. The general galactic structure appears largely undisturbed, indicating minimal signs of major merging or tidal disruption.