The observed galaxy appears as a disk galaxy, viewed nearly edge-on. The galactic disk appears elongated with a bright, seemingly smooth bulge, showing an elliptical shape. The bulge exhibits a yellowish-orange color, suggestive of an older stellar population. Dust lanes are visible in the disk, obscuring some of the light from the bulge and possibly causing reddening of background light. A distinct red emission is visible within the plane of the disk. The edge-on orientation obscures much of the disk's spiral structure, preventing more detailed morphological classification. The galaxy displays no obvious signs of a major ongoing merger, but the presence of the disk may indicate a prior interaction.