The galaxy presents as a relatively small, somewhat amorphous structure. It displays a flattened, disk-like morphology, viewed at a significant inclination. The central region is brighter and more concentrated. Moving outward, the galaxy exhibits a decrease in luminosity, transitioning into a faint, diffuse halo. Faint structure with hints of spiral arms can be seen, with a slightly blue tint indicative of ongoing or recent star formation. A single region of more intense blue color is visible. The overall appearance suggests a galaxy with moderate levels of star formation activity and a significant gas content. There is some indication of minor gravitational disturbance, but not of a major merger event.
