The galaxy presents as a diffuse, centrally concentrated object. It appears to be undergoing a major merger, as evidenced by the highly irregular morphology. There are multiple distinct clumps of light, likely representing the merging nuclei of the progenitor galaxies or regions of enhanced star formation triggered by the interaction. A tidal tail or bridge is not apparent. The object appears to be relatively compact, with the majority of the light concentrated in a region about 5 arcseconds in diameter. The color index suggests a moderately red population.