The galaxy presents as a somewhat elongated, disk-like structure, potentially viewed at an oblique angle. It exhibits a color gradient, transitioning from bluer hues at one end to warmer, yellower tones towards the central region. This may indicate varying stellar populations, with younger, hotter stars populating the bluer regions and older, cooler stars concentrated toward the center. There appears to be a separate clump of stars towards the bottom right. It cannot be determined from this image if it is interacting with the galaxy. The galaxy appears relatively smooth in overall structure with no obvious spiral arm features. It exhibits signs of possible minor disturbance. The galaxy exhibits significant star formation, as suggested by its color, but the rate is likely not extreme. The overall morphology suggests it is not undergoing a major merger but possibly experiencing a minor interaction or internal disturbance.
