The galaxy presents as a diffuse, relatively small object. Based on the available color information, the galaxy's emission appears to be primarily in the g and r bands, with faint emission possibly in the z band. The morphology is complex; evidence suggests a disrupted structure, with indications of potential tidal features or interactions. There are no clear signs of a spiral structure or a defined central bulge. The light distribution is irregular, suggesting uneven star formation or dust obscuration. The galaxy's overall appearance points toward either a late-stage merger or a galaxy undergoing significant tidal disruption.
