The galaxy exhibits an overall amorphous structure, appearing highly disturbed and asymmetric. There is a dominant, somewhat diffuse yellow-orange core, suggesting a significant population of older stars or dust obscuration. This is adjoined with a bright, compact, blueish region, which may indicate an area of active star formation or a tidal feature resulting from an interaction. There also appears to be a second, redder core or region of increased density. The object shows indications of possible ongoing or recent merger activity. The overall shape leans toward circular.
