This galaxy presents as a relatively smooth and elongated structure. Its shape is predominantly cigar-shaped, with a high axial ratio, indicating a highly inclined or edge-on disk. The light distribution suggests a central bulge or core region, which seems slightly brighter compared to the rest of the galaxy. Subtle color gradients are visible, possibly indicating variations in stellar populations and dust content across the disk. There is a general lack of distinct spiral arm structures, but the slight color variations suggest internal structure. The galaxy appears to be largely undisturbed, showing no obvious signs of recent major mergers or interactions with other galaxies. There may be minor disturbances, but the primary impression is of an isolated disk system.
