The galaxy presents as a diffuse, centrally concentrated object. It appears to be undergoing a significant interaction or merger event. There is evidence of tidal disruption, with extensions or tails visible emanating from the main body of the galaxy. The galaxy exhibits a mixed color profile; the central region appears more yellow, potentially indicating an older stellar population, while the extended features show a bluer hue, perhaps suggesting ongoing or recent star formation triggered by the interaction. The overall morphology is highly disturbed and irregular, far from a settled, disk-like or elliptical shape. There is a presence of dust obscuring some regions which adds complexity. The light is mostly compact, with a diameter of around 8 kpc.
