The galaxy appears as a diffuse, moderately bright object with a slightly irregular morphology. The overall color appears to be trending towards the bluer end of the spectrum, especially when considering the galaxy's distance. There is some suggestion of disturbance in the overall structure, possibly indicative of tidal interactions or a recent minor merger event. The light profile seems relatively smooth, yet there appear to be some localized regions of enhanced emission. These could potentially be regions of active star formation.
