The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy viewed at a significant angle. The light distribution appears relatively smooth, with a possible slight concentration towards the center, indicating a bulge component. There is a hint of dust lanes or spiral arms present, but the image resolution limits definitive identification. The galaxy's color is generally blue-ish, indicating recent star formation, but there are also some redder patches, which could be indicative of older stellar populations or dust extinction. Overall, the galaxy appears to be in a relatively isolated state, showing no obvious signs of ongoing merger activity or major tidal disturbances.
