The galaxy presents as a flattened, disk-shaped structure, viewed nearly edge-on. A prominent central bulge is observed, exhibiting a smooth, concentrated light distribution, appearing yellow-orange. The disk itself appears relatively thin, with a mottled texture suggesting some star formation activity. There is a slight hint of dust lanes within the disk, obscuring some of the starlight. The overall color profile suggests a galaxy dominated by older stellar populations, especially within the bulge, with some regions exhibiting bluer hues indicative of younger stars. No signs of recent major merger activity are observed, although there is a hint of a minor disturbance.
