The galaxy presents as a diffuse object with a complex morphology. Its color is predominantly green, with an estimated effective radius of approximately 2 arcseconds. There appears to be a central, slightly brighter region, surrounded by a fainter extended halo. Faint disturbances are present which may indicate a recent minor merger event. No strong spiral arm features are apparent. The galaxy exhibits a non-negligible fraction of merger signatures which could indicate the system is undergoing a merger.
