The galaxy exhibits a notable degree of interaction or merger activity. It presents as two distinct, yet closely associated luminous regions. The morphology suggests an intermediate stage of merging, characterized by noticeable disturbance but not yet a fully coalesced single structure. One region appears rounder with a smoother profile, possibly representing the remnant core of a progenitor galaxy. This structure appears more yellow in color. The other region seems more elongated and somewhat irregular, and redder, suggesting a more disrupted state. A faint bridge of material appears to connect the two regions. The color variation observed, with a generally redder hue overall, potentially signifies an older stellar population and ongoing star formation.