The galaxy appears to exhibit a morphology somewhere between smooth and exhibiting features. The light distribution suggests a possible central bulge or core region, presenting a relatively concentrated area of luminosity with a slight blue tint. This is followed by a less concentrated region with a yellow tint. The overall shape appears somewhere between round and elongated. It appears that there could be a merging event occurring. There is evidence of disturbance and a possible tail-like structure extending from the central region, indicating potential tidal interactions or ongoing merger activity with another galactic body. 
