The galaxy presents a somewhat amorphous morphology, with a central, brighter region surrounded by several less concentrated clumps of luminosity. The distribution of light suggests a system undergoing significant gravitational interaction or merger activity. The overall color appears to be yellowish-orange, possibly indicating an older stellar population. There appears to be a noticeable lack of distinct spiral arm structure or a well-defined disk. The shape of the galaxy is more or less round. A portion of the features appear to be merging with the main body of the galaxy. Overall the galaxy appears to be undergoing some kind of interaction.
