The galaxy appears to be an interacting system or undergoing a merger. One component is a bright, relatively spherical object with a yellowish hue, potentially indicative of an older stellar population. Adjacent to this is a more diffuse, bluish region, suggesting the presence of younger, hotter stars and ongoing star formation. The overall shape is irregular, with possible tidal features or disturbances extending from the central region. There is evidence of significant morphological disturbance. The galaxy is relatively large in apparent size, and is likely a massive system. Its low rate of star formation suggests that it has mostly depleted its gas and is likely an older galaxy.
