The galaxy exhibits a generally amorphous morphology, appearing irregular and without a well-defined structure. It possesses a central, somewhat brighter region that could be considered a core, though it lacks sharp delineation. A diffuse, extended halo of fainter material surrounds the central region. There are indications of possible tidal features or distortions, suggestive of past or ongoing gravitational interaction with another galaxy, however, these are very faint. Color gradients are present, with the central regions displaying a relatively redder hue compared to the outer edges, which exhibit bluer tones. This difference might indicate differing stellar populations or dust content within the galaxy. Overall, the galaxy's structure is significantly disturbed, implying a complex formation history.
