The galaxy exhibits a prominent, centrally concentrated bulge, surrounded by a well-defined disk. The spiral arms are clearly visible and loosely wound, with a noticeable two-armed structure. A weak bar feature appears to be present in the central region. The disk shows some clumpy structure indicating regions of active star formation. There is no indication of significant morphological disturbance or ongoing major mergers, but there may be a minor disturbance visible. The galaxy is observed at a moderate redshift.
