The observed galaxy presents as a system undergoing a significant interaction or merger. The overall morphology is highly disturbed, exhibiting irregular features and a lack of clear spiral arm structure or a well-defined elliptical shape. Light distribution is uneven, with multiple bright, concentrated regions suggesting the presence of distinct nuclei or intensely star-forming clumps. Tidal tails or bridges of material appear to extend outward, further indicating gravitational interaction. The color distribution is varied, with reddish hues suggesting older stellar populations and dusty regions, while bluer colors may indicate areas of active star formation. The system is estimated to be of substantial size, exhibiting a luminosity that suggests a relatively high mass.
