The galaxy exhibits an overall disturbed morphology, indicative of an ongoing or recent interaction. The central region presents a bright, yellowish core suggesting an older stellar population. This is enveloped by a larger, more diffuse region of bluish light, which might signify areas of more recent star formation. A significant portion of the galaxy's light appears somewhat smooth. The galaxy appears to be roughly in between rounded and cigar shaped. Evidence points to this system possibly being a late-stage merger.
