The galaxy presents a distinct spiral morphology, exhibiting a flattened disk structure. The spiral arms are clearly visible, and appear to be tightly wound around the galactic center. There is a noticeable central bulge component, but it does not dominate the overall structure, suggesting a modest size relative to the disk. The disk itself shows some degree of inclination with respect to our line of sight. The luminosity appears to be greatest in the central region, gradually decreasing outward towards the edges of the disk. There is possible evidence of active star formation within the spiral arms. There is no immediately obvious indication of a major ongoing merger event, though minor disturbances in the disk cannot be ruled out.
