The galaxy presents as a system possibly undergoing a merging event or exhibiting strong tidal interactions. It appears to be a complex structure with three distinct luminous components. The brightest component is centrally located and exhibits a smooth morphology, suggestive of an elliptical galaxy or the bulge of a spiral galaxy. It possesses a yellowish hue, potentially indicating an older stellar population. To the right of this central component, there is a second, less defined luminous area, which could be another interacting galaxy or a region of enhanced star formation triggered by the interaction. A third distinct object below the central galaxy is visible with a similar yellowish colour.

The overall shape of the system deviates significantly from a regular elliptical or spiral morphology, indicating a disturbance in its gravitational equilibrium. The presence of distorted features points towards ongoing gravitational interactions, potentially leading to a future merger. The colour distribution within the system suggests variations in stellar populations and potentially varying levels of dust obscuration throughout the galaxy.
