The galaxy presents a morphology indicative of a possible merging event or interaction. The light distribution appears disturbed, showing an elongated shape with what seems to be two possible distinct central concentrations of light, suggesting the presence of two nuclei. These two "bulges" appear connected by fainter regions, giving the galaxy an overall irregular shape. The color profile seems fairly uniform with an overall yellow-ish color in the central areas. The outer regions are more faint. There appears to be no clear disk component, the galaxy appears mostly spheroidal.
