The object appears to be a galaxy, exhibiting a non-smooth, disturbed morphology. The light is dominated by yellowish-orange hues, suggesting an older stellar population, or significant dust obscuration of any younger stars. There is a suggestion of a tidal tail or bridge extending from the main body of the galaxy, hinting at an ongoing or recent interaction with another galaxy, or possibly an ongoing merger. There appear to be multiple knots of higher luminosity within the galaxy, which could correspond to regions of increased star formation activity, or potentially the cores of merging galaxies. The object does not present a clear disk structure, but this may be due to the viewing angle or the advanced stage of the merger. The overall impression is of a galaxy undergoing significant disruption, likely from gravitational interaction.
