This galaxy presents an irregular morphology, exhibiting a disturbed or merging structure. The light distribution is not smooth and appears to be composed of at least two distinct bright, compact regions that are connected by a faint stellar bridge. The color profile shows a bluer hue in these bright regions, suggesting the presence of young, hot stars indicative of recent or ongoing star formation. The overall structure indicates a potential interaction or merger event, which is disrupting the galaxy's morphology and triggering star formation. The extended, fainter light surrounding the core regions may be indicative of tidal tails or debris associated with the interaction, which are not well defined.
