The galaxy appears to be composed of two distinct, luminous components, possibly undergoing a merger or interaction. The larger component exhibits a smoother, more diffuse light distribution with a yellowish hue, suggesting a population of older stars. The smaller component has a more concentrated, orange-tinted emission, potentially indicative of on-going star formation or a denser stellar population. There is a clear bridge of light between the components. The overall morphology is disturbed, deviating from a regular elliptical or spiral structure, which supports the possibility of an interaction or recent merger event.
