The galaxy exhibits a merging morphology, with what appears to be two distinct galactic nuclei closely interacting. One nucleus displays a yellowish-orange hue, suggestive of an older stellar population and a relative lack of active star formation. The second nucleus presents a bluish color, hinting at a younger stellar population and ongoing star formation. The overall shape of the system is irregular, showing signs of tidal disruption and gravitational interaction. The galaxy has a fairly round appearance, though noticeable disturbances are present due to the on-going merger. There is a faint stellar halo surrounding the main body of the galaxy. The colors of this galaxy are shifted into the red slightly due to it being a distant galaxy.
