The observed galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is evidence of a faint disk structure, though the angle prevents a clear classification. The galaxy is characterized by an asymmetrical morphology. One side of the galaxy is more prominent and exhibits a brighter concentration of light, indicating a potential density variation within the galactic structure. There is a slight blue tint to the galaxy, indicative of active star formation. Faint hints of spiral arms can be seen, but these features are not highly defined. There is an ambiguous morphology suggesting it could be experiencing a minor disturbance.
