This galaxy presents as a system with apparent signs of disturbance or interaction. The overall morphology appears somewhat irregular. The light distribution of the galaxy presents itself as being between a smooth and featured morphology, with a dominant central bulge and hints of a disk structure. It does not appear distinctly round. The shape of the bulge is elongated and somewhat cigar shaped. Patches of what appear to be active star forming regions with bluer light can be identified towards the edges of the galaxy. It is exhibiting activity suggesting a moderate rate of star formation. The redshift of the galaxy indicates that it is at a considerable distance. There are signs of tidal interactions and potentially a merging event. The presence of two distinct components of the galaxy suggest there are two components, or it could be one galaxy experiencing a strong tidal disruption.
