The galaxy presents as a somewhat diffuse, bluish object. Its morphology suggests a system that is either undergoing a merger or experiencing significant tidal interactions. The central region is brighter, hinting at a possible nucleus or concentration of older stars, though it is not sharply defined. There are hints of disrupted structures with a possible tidal tail or bridge extending outwards. The blue color suggests the presence of recent star formation, particularly in the brighter regions. The overall shape appears elongated, with no clear spiral arms or well-defined disk visible. There are also some faint clumps of light that may be star forming regions or remnants of a smaller galaxy, or simply be caused by background noise.
