The galaxy presents as a disturbed system, exhibiting morphological characteristics indicative of an ongoing or recent merger event. The primary visible structure shows a distorted, elongated form, with a noticeable tidal tail extending outwards. The light distribution within the main body appears uneven, and there is a lack of defined spiral arm structure. Multiple bright knots are visible embedded within the galaxy, suggesting regions of active star formation, potentially triggered by the interaction. The red-optical light appears concentrated in certain areas, possibly indicating older stellar populations or significant dust obscuration. The overall color is dominated by redder light, with some green-yellowish emission near the central regions. Overall, the object exhibits characteristics of a merging system with ongoing star formation and a significantly disrupted morphology.
