The galaxy exhibits an elongated, cigar-shaped morphology, suggesting it is likely an edge-on spiral or a lenticular galaxy. There appears to be a relatively smooth light distribution within the galaxy's main body, although there may be some subtle features or a hint of a disk-like structure. Some minor disturbances might be visible, but these are fairly subtle and do not indicate a recent major merger. The light from the galaxy is predominantly in the blue-green, suggesting moderate active star formation. There is little or no presence of dust. The size appears to be of intermediate value, approximately 7.6 kpc across.
