The galaxy presents as a diffuse, irregularly shaped object, with a noticeable blue tint. The central region appears slightly brighter and more condensed compared to the outer edges, suggesting a possible core or bulge. The galaxy lacks a well-defined spiral structure; instead, it exhibits a more amorphous, disturbed morphology. There are hints of tidal features or extended arms extending from the main body, indicating potential past interactions or ongoing mergers with smaller companions. The galaxy's color suggests a presence of relatively young, hot stars, possibly induced by the aforementioned interactions. Overall, the galaxy appears to be in a state of dynamic activity, possibly evolving due to internal or external factors.
