The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. The spiral arms are clearly visible, displaying a tightly wound morphology. We can observe a well-defined central bulge region, smaller relative to the disk. The presence of a bar-like structure is moderately apparent within the central region. The arms show some level of patchiness, hinting at active star formation regions with associated dust lanes. Overall, the galaxy appears well-formed and relatively undisturbed.
