The galaxy presents as a relatively large, disk-shaped structure, viewed at a high inclination. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, the disk displays a bluer tint, indicative of ongoing star formation. The arms are not well-defined or show significant irregularities, possibly due to the viewing angle, or because of the morphological features. Faint wisps of material extend beyond the main body of the galaxy, suggesting possible tidal interactions or recent mergers, although the overall structure does not appear significantly disrupted. The galaxy is of intermediate redshift, though details cannot be distinguished.
