The galaxy presents a somewhat smooth, disk-like morphology, and is observed nearly edge-on. There is a noticeable central bulge that appears brighter and more concentrated. The disk component shows a subtle color gradient, transitioning from a bluer hue toward the outer edges to a slightly redder tint near the central bulge. There is no evidence of significant merger activity or major tidal disturbances. The galaxy appears to be a relatively undisturbed system.
