The galaxy presents as a flattened, elongated structure, consistent with a disk galaxy viewed at an oblique angle, though not perfectly edge-on. Its primary color is a pale blue, suggestive of a population of relatively young, hot stars. The luminosity is generally uniform across the structure. The features are somewhat indistinct, without clearly defined spiral arms. The disk morphology indicates a notable degree of rotational support. Some mild tidal disturbances can be observed, potentially indicating an interaction with a smaller neighboring galaxy. There is some variation in color, which implies some regions of recent or ongoing star formation. The lack of a prominent bulge suggests that the galaxy may have a relatively low-mass supermassive black hole. The overall appearance of the galaxy suggests a system with a moderate rate of star formation.
