The galaxy appears as a single, relatively smooth, centrally concentrated object with an ellipsoidal morphology. The light profile is diffuse, without strong spiral arm features. There are several features that point towards it being involved in some sort of interaction. There is a second, smaller, nearby object that may be another galaxy. The image shows the galaxy to have a redder hue. This suggests an older stellar population, and possibly a relatively low rate of star formation. There is no obvious dust lane structure visible. The object appears fairly rounded. A slight visual asymmetry or warping is present in its shape. The morphology suggests that the object has potentially undergone a recent minor merger event or is experiencing tidal interactions, although a major disturbance or full merger cannot be ruled out.
