This galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The galaxy appears to be composed of two distinct, roughly spherical components or nuclei, with a connecting bridge of fainter luminosity material between them. One of these components shows a reddish hue, while the other presents a more yellowish to golden coloration. The overall light distribution suggests a relatively smooth structure with hints of disturbance, but with a dominant fraction showing a smooth nature. The galaxy's light output is relatively high, indicating a substantial stellar population and possibly ongoing star formation activity. There are no clear spiral arm features, but the shape is distorted from a regular elliptical or spiral form. 
