The galaxy presents as an interacting system, characterized by significant morphological disturbance. There is a primary, diffuse component with a smooth appearance and a distinct yellow hue, suggesting an older stellar population. It is accompanied by a secondary component that is more compact and exhibits a redder color index, potentially indicating dust obscuration or a difference in stellar population. A clear tidal feature is not readily apparent, however the interaction suggests an ongoing or recent merger. The overall shape is quite irregular and suggests an unrelaxed system. Given the color differential between the components, we could expect a difference in mass between the two components, with the redder one being less massive. This is more than likely a merging system, with the primary galaxy in the process of absorbing the secondary object.
