The galaxy presents as a somewhat smooth, centrally concentrated object with a hint of disk-like structure. A dominant, bright, yellowish core is apparent, possibly indicating an older stellar population or significant dust obscuration in the central region. Adjacent to this core is a very bright, more circular object with a greenish color, potentially indicative of active star formation. Overall, the galaxy exhibits a moderate degree of disturbance, with evidence suggesting a potential interaction or merger event might be occurring. The galaxy exhibits a relatively compact size.
