The galaxy appears as a flattened, disk-shaped structure viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a spheroidal morphology. There is little indication of strong spiral arm structure or significant dust lanes. The galaxy has an orange hue, suggesting an older stellar population. Faint asymmetrical extensions are observed at both ends of the disk. These faint structures could indicate tidal interactions or past mergers, although no major disturbance to the galaxy’s overall structure is apparent. Overall, the galaxy presents a smooth appearance, with no apparent ongoing intense star formation.
