The galaxy presents as a relatively compact object with a smooth, diffuse appearance. It appears to be undergoing a significant interaction or merger. The morphology exhibits a somewhat distorted shape, potentially indicating gravitational disturbances. The color profile suggests a mix of stellar populations, with a dominant yellowish hue indicative of older stars. Patches of bluer light are present in several areas, hinting at localized regions of active star formation. The estimated size suggests a galaxy of substantial physical extent.
