The galaxy presents an irregular morphology, lacking a clearly defined structure such as spiral arms or an elliptical shape. It exhibits a diffuse, elongated form spanning an approximate angular diameter of ~13 arcseconds. A notable feature is the presence of disturbed features, suggesting potential gravitational interactions or recent merger events. The color gradients indicate varying stellar populations or dust distribution across the galaxy. A bluer region appears in one area, potentially indicating ongoing star formation. Overall the galaxy appears to be undergoing significant disruption, suggestive of a dynamic and evolving system. 
