The galaxy presents a morphology that is neither definitively smooth nor clearly disk-like. Its overall structure appears somewhat amorphous. There is a hint of a central bulge, but it is not well-defined. Faint tidal tails are potentially visible. The galaxy's light distribution exhibits a redder core, with bluer regions extending outwards. The presence of these bluer regions may indicate ongoing or recent star formation. The galaxy shows some evidence of minor disturbances in its structure, which could suggest a past or ongoing interaction with another galaxy. It is difficult to fully ascertain the nature of these disturbances based on the image.
