The galaxy appears as a centrally concentrated object with a generally elliptical morphology. The light distribution is relatively smooth and lacks prominent spiral arm structures. A hint of bluer hues emanate from the galaxy's core. The object displays no significant tidal tails or obvious signs of a major ongoing merger event, though some level of disturbance is indicated by its irregular shape, indicating a possible merger event or gravitational interaction. Overall, it presents as a somewhat disrupted system.
