The galaxy presents as a complex, potentially interacting system. It appears to be composed of multiple components or distinct regions of activity. The brightest region exhibits a concentration of light with a slightly redder hue, possibly indicating an older stellar population or significant dust obscuration. An adjacent, somewhat fainter region displays a bluer color, suggesting ongoing or recent star formation. There is a suggestion of disturbed morphology, possibly due to tidal interactions with another galaxy, although without higher resolution, this remains speculative. Overall, this appears to be a galaxy with a diverse stellar population and possibly undergoing a merger or significant gravitational disturbance.
