The galaxy presents a disturbed morphology, possibly indicative of an ongoing or recent interaction. The main body of the galaxy appears somewhat elliptical, with a smooth central region. There are hints of diffuse, extended light surrounding the core. A distinct feature is the presence of multiple distinct knots or clumps of light surrounding the galaxy, indicating ongoing or recent star formation. The colors of these star forming regions appear redder than the rest of the galaxy. The galaxy exhibits a redder hue, suggesting an older stellar population.