The galaxy presents as a single, extended object with a somewhat amorphous shape. Its morphology is neither clearly elliptical nor spiral. The light distribution suggests a complex structure, possibly involving an ongoing or recent merger event. There are some slight irregularities. The central region appears brighter and more condensed than the surrounding areas. There is evidence for disturbed features within the central region. The color appears to be redder overall, indicating the presence of an older stellar population and potential dust obscuration, and the object has moderate brightness. The galaxy appears to be a substantial mass. Star formation may still be ongoing, but not at high levels.
