The galaxy presents a morphology indicative of a possible ongoing merger. The primary body exhibits a somewhat amorphous shape, lacking a well-defined spiral structure or elliptical form. There is a possible second object slightly offset from the primary body that appears to be interacting gravitationally.

The color profile suggests a mix of stellar populations, with some regions exhibiting bluer hues, potentially indicating areas of active star formation, and other regions showing redder tones, consistent with older stellar populations. The surface brightness distribution is relatively uneven, further supporting the likelihood of a disturbed system, potentially due to tidal interactions associated with the apparent merger. Light from this galaxy has been redshifted indicating its distance and relative motion away from us.
