The galaxy exhibits an irregular morphology, appearing as a disturbed system. The structure is dominated by what appears to be a major ongoing merger event, rather than displaying features of a spiral or elliptical galaxy. There are at least two distinct luminous components, suggesting the nuclei of the merging galaxies, with a disturbed, diffuse structure.

The color gradients suggest active star formation, particularly in the regions of higher luminosity. A tidal tail or bridge appears to extend from one of the main components, indicative of gravitational interactions. The system shows a redder color profile overall, hinting at a developed stellar population, with areas of bluer emission that may indicate ongoing star formation.
