The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure oriented nearly perpendicular to the line of sight. A central bulge is clearly visible, appearing bright and concentrated. The bulge exhibits a more diffuse, rounded morphology. The disk itself demonstrates a smooth appearance, with minimal indication of distinct spiral arm structures from this viewing angle.

A dust lane appears to bisect the galaxy, darkening the midplane and obscuring light from the stars behind it. The galaxy appears asymmetric, suggesting a possible gravitational interaction or recent merger event that is causing the shape. The disk extends a considerable distance from the central bulge, with a length that is visually several times larger than the bulge's diameter. The color profile transitions from a yellowish hue at the bulge to a bluer tint within the disk.
