The galaxy presents as two distinct, luminous components. One component appears to be more concentrated and brighter, exhibiting a bluish-white hue, suggesting a population of hot, young stars. The second component is less concentrated, with a more diffuse appearance and a yellowish color, potentially indicative of an older stellar population. There appears to be some disturbance or interaction between the two. The overall morphology points to an ongoing or recent merger event. There are no apparent spiral arms or other distinct features; the light is generally smooth, indicating a possible evolved system.
