The galaxy exhibits a morphology suggestive of an ongoing or recent merger. The light distribution appears disturbed, with an elongated structure and two distinct, bright central regions or nuclei, possibly representing the cores of the merging galaxies. Overall the color is relatively red, suggesting an older stellar population with relatively low star formation. There is some suggestion of blue areas but its low surface brightness suggests that star formation is suppressed. The primary component appears smooth with significant disruption.
