The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, concentrated light profile that fades into the surrounding disk. The color of the bulge suggests an older stellar population. The disk, while tightly wound, shows some subtle indications of structure. No obvious signs of active star formation are visible within the disk. The overall symmetry of the galaxy appears relatively undisturbed, with no major tidal features or signs of recent merger activity immediately apparent. The galaxy exhibits a moderate redshift.
