The galaxy presents as a flattened, elongated structure, approximately 5 arcseconds in its longest dimension. The overall morphology appears to be disk-like. The light is primarily in the green part of the spectrum. There is a small, nearly spherical, very bright object positioned close to one end of the disk. Its proximity suggests a possible interaction or tidal disturbance. No strong spiral arm structures are immediately apparent. While the main body of the galaxy appears relatively smooth, there might be minor disturbances. However, it does not appear to be undergoing a major merger.
