The galaxy exhibits a complex morphology, presenting characteristics suggestive of an ongoing or recent merger event. Two distinct, luminous components are discernible. The primary component displays a more diffuse, greenish-yellow hue, while the secondary component exhibits a more concentrated, reddish-orange color. The overall structure is disturbed, deviating from a regular elliptical or spiral form. The observed colors imply differing stellar populations and dust content within the individual components, with the redder component potentially harboring older stars and/or being more obscured by dust. The system appears relatively compact, yet possessing a significant luminosity, indicative of a substantial stellar mass and potentially high star formation activity. The system does not appear to show any clear spiral arms or a well defined disk.
