The galaxy appears to be relatively compact with a bright, concentrated central region. The morphology suggests a disturbed system, possibly the result of a minor merger. There is a discernable plume or tidal tail extending from the central region, indicating gravitational interaction with another object. This plume is noticeably redder in color than the main body of the galaxy. The main galactic body itself presents a somewhat irregular shape, with some indications of faint, diffuse features that could be spiral arm fragments or disrupted galactic structure. The overall color profile suggests a mix of stellar populations, with some areas exhibiting bluer hues indicating ongoing or recent star formation, while others appear redder indicating older stellar populations or dust obscuration.
