The galaxy appears to be a faint, disturbed system with an angular size of approximately 3 arcseconds. It displays a somewhat amorphous morphology, lacking a well-defined nucleus or spiral arm structure. There appears to be a primary body of stars, with hints of tidal tails or extended debris fields. Irregular features are present, including possible dust lanes and regions of enhanced star formation, especially in the North end of the galaxy. These features contribute to an overall clumpy or fragmented appearance. Light is bluer in the northern most regions and more red in the southern most regions. The morphology suggests a possible interaction or merger event that has disrupted the galaxy's original structure. 
