The galaxy presents as a relatively smooth, disk-shaped structure with a noticeable central bulge. The overall color of the galaxy suggests a mix of stellar populations, but with an emphasis on younger, bluer stars.

The disk exhibits a faint but distinct spiral arm structure. Patches of brighter, bluer regions within the spiral arms hint at ongoing star formation activity. The core appears slightly more red, potentially indicative of an older stellar population or increased dust obscuration.

The overall morphology appears relatively undisturbed, with no obvious signs of a major merger event. There is a slight elongation to the galactic disk.
