The galaxy presents a morphology suggestive of a merging system, exhibiting two distinct, luminous components. The upper component appears more yellow, indicating an older stellar population with less ongoing star formation. The lower component is noticeably bluer, indicative of more recent or ongoing star formation. The components are connected by a faint, diffuse structure. The overall shape of the system appears somewhat irregular and disturbed, consistent with the interaction of two galaxies. There may be tidal tails or bridges present, but it is hard to assess due to image quality.
