The galaxy exhibits a distinct disk-like morphology, appearing somewhat elongated on the plane of observation. A subtle central bulge is visible, though it does not dominate the overall structure. The disk is not entirely smooth; there is evidence of some irregular features and possible disturbances within the galactic plane. The color distribution suggests variations in stellar populations. A somewhat blue hue is present in certain regions which may suggest the recent formation of stars. The shape is reasonably organized, though asymmetries indicate potential minor gravitational interactions or internal processes. There's a possibility that there may be a hint of distortion due to a merging event, although it is fairly minor.
