This galaxy appears to be undergoing a significant interaction or merger event. The morphology suggests the presence of at least two distinct components or nuclei. One component is brighter and more centrally concentrated, exhibiting a yellowish-white hue. The other is slightly less bright and less centrally concentrated. There appears to be a tidal tail extending from the merging galaxy, or possibly other interacting dwarf galaxies. Light from each object is generally smooth, although the interaction may be obscuring further details. The object as a whole is somewhat oblong in shape, though the specific structure is difficult to determine due to the interaction. There appears to be some dust or regions of star formation that give the galaxies a reddish hue.
