The galaxy appears to be undergoing a major merger event, with a disturbed morphology. Two distinct nuclei are visible, one significantly brighter and more prominent than the other. Both nuclei exhibit a yellowish-orange hue, potentially indicative of an older stellar population and reduced ongoing star formation. The galaxy's overall light profile is smooth, likely a result of the advanced stage of the merger, where tidal features are not readily apparent in this image resolution. There is a suggestion of a more diffuse halo around the central region, but the faintness limits certainty. The system is approximately round with a possible cigar shape morphology.