This galaxy presents as a flattened, disk-like structure viewed nearly edge-on from our vantage point. The central region exhibits a high degree of luminosity, appearing almost uniformly bright and slightly blue-tinted, suggestive of a dense stellar population. Moving outward from the core along the galactic plane, the intensity decreases gradually. The outer regions of the disk display a dusty, brownish-orange hue. The lack of distinct spiral arms or irregular features indicates either a smooth, well-mixed disk or obscuration by dust. Overall, the galaxy exhibits a relatively symmetric and undisturbed morphology. There are no obvious signs of interaction or recent merger events.
