The galaxy appears to be a spiral type, with a prominent disk structure. Two major spiral arms are discernible, extending outwards from a central bulge. The winding of the spiral arms appears to be of medium tightness.

The central bulge is moderately sized, exhibiting a yellowish hue, which suggests a population of older stars. The disk shows bluer regions indicative of ongoing star formation, particularly along the spiral arms, which also exhibit areas of dust obscuration. There's a hint of some disturbance in the morphology, but overall the galaxy maintains a relatively coherent structure. No obvious signs of a strong bar structure are apparent. The disk is viewed at a significant angle from face-on.
