The galaxy appears to be a relatively faint, disk-shaped system. It exhibits a generally smooth morphology with some subtle indications of spiral arm structure; however, these features are not sharply defined. The galaxy appears to be experiencing some kind of disturbance due to the slightly asymmetrical shape. The color profile is predominantly blue, suggesting the presence of younger, hotter stars, though this blueness is more prominent in some regions than others. The central bulge is not particularly prominent. There are no well-defined dust lanes visible. Overall, the galaxy's visual characteristics suggest ongoing, albeit perhaps not intense, star formation within its disk.
