The galaxy presents as a merging system or interacting pair. It appears to be composed of two distinct, bright components. The larger, more northern component exhibits a diffuse, somewhat smooth morphology with a bluish tint, suggesting ongoing star formation or a younger stellar population. The southern component is smaller, more concentrated, and possesses a yellow-orange hue, indicative of an older stellar population or dust obscuration. A faint bridge of material seems to connect the two components, hinting at tidal interactions. The overall shape of the system is irregular, with no clear spiral arms or defined disk. This morphological disturbance is consistent with an ongoing merger event. The system exhibits a moderate luminosity, suggesting a substantial stellar mass. Overall, this galaxy shows signatures of a dynamic system undergoing significant gravitational interactions.
