The galaxy presents a disk-like morphology with a relatively low inclination with respect to our line of sight. Faint spiral arm structures are suggested within the disk, but no distinct, well-defined spiral arms are apparent. There's a subtle central bar-like structure with moderate prominence. The bulge appears relatively small or even non-existent; there is no readily distinguishable bulge component. The overall color of the galaxy appears to be bluish, indicating a younger stellar population and active star formation. There are a couple of regions of more intense blue coloration, implying concentrated areas of active star formation. The galaxy does not appear to be undergoing any major mergers, though there may be a minor disturbance or interaction hinted at by the asymmetry of the outer disk. The galaxy exhibits a somewhat flocculent or patchy structure, particularly in the disk.
