The galaxy appears to be a spiral galaxy viewed at an oblique angle. Its morphology suggests the presence of well-defined spiral arms originating from a central bulge region. The arms appear to be relatively tightly wound. There is a hint of a bar-like structure intersecting the central bulge. Patches of star forming regions, implied by the varying colors, are observed along the spiral arms. The galaxy is likely of an intermediate size and mass. Overall, it presents a classic spiral structure with evidence of ongoing star formation.
