The galaxy presents an edge-on disk morphology. A prominent bulge dominates the central region, exhibiting a yellowish hue, suggesting an older stellar population. The bulge appears to be rounded. Faint bluish extensions can be observed on either side of the central bulge, possibly representing the spiral arms of the disk. These arms do not appear well-defined, indicating that the galaxy could have a smooth disk. There is no visible sign of any major disturbances or ongoing mergers. The overall structure suggests a relatively undisturbed system with a stable configuration.
