The galaxy presents an irregular morphology. It appears to be undergoing a major merger event, with significant tidal disturbances visible. The core region displays a moderate level of central condensation, but the overall shape is highly distorted. There's evidence of ongoing star formation, particularly in areas of interaction between the merging components, as indicated by the presence of bluer regions. A significant portion of the galaxy has a smoother, more diffuse appearance, possibly representing an older stellar population. The overall color indices suggest a substantial population of evolved stars, but the bluer knots indicate pockets of more recent star formation. The system is approximately 8 kiloparsecs across. The estimated stellar mass is substantial.
