The galaxy presents a diffuse, somewhat irregular morphology. It appears to be a relatively low-mass system, exhibiting a faint, blue-ish hue that may indicate ongoing star formation. There is no distinct nucleus visible, but rather a gradual increase in luminosity towards the central region. The galaxy appears to show signs of a merger event, or a significant interaction with another galaxy. Evident of a major disturbance. There is some irregularity or disturbances.
