The galaxy presents a discernible disk structure with evident spiral arms. The arms appear somewhat tightly wound around a central bulge region. The bulge exhibits a moderate size, contributing substantially to the galaxy's overall luminosity. The galactic disk displays a mottled texture, indicative of ongoing star formation. The spiral arms themselves are not perfectly symmetrical, hinting at possible gravitational interactions or internal disturbances. Some degree of asymmetry is observable within the spiral arm structure. There is evidence suggesting minor tidal disruption occurring. The central bulge shows a smooth color gradient toward the galaxy's center. The disk is viewed at an angle closer to face on. The color of the galaxy ranges from yellow to blue.
