The observed galaxy appears to be an interacting system. The primary galaxy exhibits a prominent bulge, approximately half the size of the overall system, with a moderate concentration of light toward the center. Faint spiral arm structures are visible emanating from the central region. The color profile suggests ongoing star formation.

A second distinct but smaller galactic component is observed close to the primary galaxy. A tidal bridge of stellar material appears to connect the two galaxies, indicating an ongoing gravitational interaction. This interaction seems to be causing a distortion in the morphology of both galaxies, suggesting a recent or ongoing merger.

The system displays signs of a significant disturbance. The overall morphology suggests a merger in progress, rather than a stable, isolated galaxy.
