The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. There is a central bulge that appears somewhat elongated along the disk's major axis. The disk exhibits a subtle color gradient, transitioning from a bluer hue along the outer edges to a more yellow-ish white toward the central bulge. Faint indications of spiral arm structures appear within the disk. The galaxy appears to be a relatively isolated system, showing no signs of significant tidal disturbances or ongoing major merger events. Its overall morphology suggests a galaxy undergoing active star formation, particularly within the disk regions.
