The galaxy appears as an irregular, diffuse object with a slightly elongated morphology. A central, somewhat brighter region is visible, although there isn't a distinct, well-defined nucleus. The overall color is bluish, suggestive of a population of younger, hotter stars. The galaxy's structure lacks grand spiral arms or a prominent disk. Instead, its light distribution is more amorphous and patchy. There are hints of some internal substructure, potentially indicating regions of ongoing star formation. While it isn't possible to definitively classify the galaxy's morphology without higher resolution imaging, based on this image it may be experiencing a potential merging event, or an ongoing starburst.
