The galaxy appears to be an interacting system, comprised of at least two distinct components. The primary component exhibits a bluish hue, indicative of active star formation. This region appears somewhat irregular in shape. The secondary component exhibits a more diffuse and reddish appearance, suggesting an older stellar population and a relative lack of ongoing star formation. There is evidence of tidal disturbance, indicating a possible merger in progress. A significant portion of the light is concentrated centrally. The overall morphology is neither strictly elliptical nor spiral, displaying characteristics consistent with a galaxy undergoing a merger event.
