The galaxy exhibits a disturbed morphology, potentially undergoing a merger or exhibiting tidal interactions. The primary body of the galaxy appears somewhat smooth with a higher concentration of light. There is an extended arm feature on one side that is less concentrated and possibly distorted. The color appears to be a bluish hue, which suggests the presence of relatively young stars or active star-forming regions. The shape and light distribution is asymmetric. Overall, the galaxy does not present as a well-defined spiral or elliptical structure and appears to be disturbed.
