The galaxy presents as an interacting system exhibiting signs of a significant tidal disturbance. The main body of the galaxy appears to be generally smooth in texture, with a primarily elliptical morphology. The galaxy has a prominent bulge that presents as a yellowish to white hue, suggesting a substantial population of older stars. A clear disturbance in the form of an extended, bluish tidal tail extends away from the primary galaxy. The bluish color indicates the presence of younger, hotter stars within the tail. The galaxy appears to be undergoing or have recently undergone a merger or major interaction with another galaxy, producing the tidal tail feature. There is no clear dust lane present.
