The galaxy presents an elongated, disk-like morphology. Its structure appears to be generally smooth, though some indication of spiral arm structure may exist. The color gradient suggests the presence of distinct stellar populations. The central region exhibits a slight concentration of light, potentially indicating the presence of a bulge. There's a hint of a central bar structure. The galaxy appears to be actively forming stars, showing blue regions indicative of hot, young stars. Dust lanes may be obscuring some areas, giving a mottled appearance. The overall shape appears to be a result of rotation. It is a large galaxy.
