This galaxy exhibits a clear spiral morphology, presenting loosely wound arms. The central bulge appears subdued, with a moderate contribution to the galaxy's overall luminosity. A bar structure is evident traversing the galactic center, displaying a defined presence. The galaxy's disk is visible, oriented at an angle from our line of sight. Distinct color variations across the galaxy suggest varying stellar populations and ongoing star formation. Patches of bluer light are visible within the spiral arms, potentially indicating regions of active star formation. There are some signs of minor disturbances in the morphology, but there does not appear to be a major merger occurring.
