The galaxy presents as a flattened, disk-like structure, viewed at an oblique angle, but leaning more towards edge-on. It exhibits a central, bright bulge region, which appears relatively smooth and concentrated. The disk is less defined, with a somewhat diffuse appearance. There is a color gradient noticeable, with a blue hue along the outer edges of the disk, suggesting the presence of younger, hotter stars. The disk also shows hints of some irregular features or minor disturbances, but these are not pronounced enough to indicate a major ongoing merger. There is likely a moderate amount of on-going star formation in this galaxy.
