The galaxy appears as a merging system, exhibiting significant morphological disturbance. A larger, yellowish component is visible to the left, likely the primary galaxy. It displays a relatively smooth light distribution, with an elongated, somewhat diffuse profile. A secondary component, smaller and more reddish in color, is situated to the right, appearing partially merged or interacting with the larger galaxy. The overall shape is irregular, lacking a well-defined spiral structure. The color gradient suggests a mix of stellar populations, with the reddish regions potentially indicating older stars or dust obscuration, while the yellowish component may indicate intermediate aged or actively star-forming regions. There is a possible tidal feature or bridge of material extending between the two components, indicating the ongoing gravitational interaction. Overall, the galaxy appears to be in a late stage of a merger event.
