The object appears as a thin, elongated structure, suggestive of a highly inclined disk galaxy seen edge-on. There is a distinct color gradient across the galaxy, with a bluer component concentrated towards the upper edge and a redder component primarily on the lower side. The blue color indicates the presence of younger, hotter stars or regions of active star formation, whereas the red color could be older stars or significant dust obscuration. The relatively uniform color indicates a smooth distribution of stars or other light emitting gas. Possible disturbances are noted in the structure, indicating possible minor merging events. Overall, the observed properties are consistent with that of an actively forming galaxy.
