This galaxy exhibits a disk morphology, appearing as a flattened structure. A distinct central bulge is present, exhibiting a moderate size relative to the overall disk. The galaxy shows evidence of spiral arms, though they appear somewhat flocculent and not tightly wound. A bar-like structure seems to traverse the center of the galaxy, potentially influencing the spiral arm morphology. The disk is not perfectly edge-on, allowing for some view of the spiral structure within. There is no obvious evidence of a major merger event, though some minor disturbances in the disk's symmetry can be seen, possibly indicating a minor interaction or internal dynamic process. The light distribution suggests a relatively smooth transition from the bulge to the disk, but with subtle colour variations in the disk indicating areas of star formation.
