The galaxy exhibits a disk-like morphology, but does not have a perfectly smooth appearance. Some regions are more distinct than others, suggesting possible substructure or uneven stellar distribution within the disk. There is some evidence for a spiral structure, but it is not highly defined. The galaxy appears to have a moderate bulge component. A bar structure may be present, but is indistinct. The galaxy does not appear to be undergoing a major merger, though signs of minor disturbances may be present. The galaxy shows relatively high rates of star formation. The size of the galaxy appears to be normal.
