The galaxy appears as a faint, elongated structure, characterized by a bluish hue. Its overall morphology suggests a disk-like component, although it's challenging to discern a definitive spiral arm structure. The light distribution indicates a relatively smooth profile across the galaxy, with a higher concentration of blue light suggesting ongoing star formation.

There is some indication of tidal disturbances, with asymmetry in its outer regions and a slightly distorted shape. The galaxy's color suggests a significant population of young, hot stars, which indicates active star formation. The lack of a prominent central bulge suggests a lower stellar mass within the galactic nucleus. Given the disturbances, it is possible the galaxy is undergoing a minor merger.
