The galaxy presents as a system undergoing a significant merger. The morphology is highly disturbed, with no readily discernible spiral arms or elliptical structure. The primary component appears as a diffuse, luminous region, exhibiting a greenish hue that may indicate elevated star formation activity. Embedded within this region are several compact, reddish knots which are likely sites of concentrated star formation, possibly triggered by the interaction. A secondary, more compact component sits closely, displaying a yellowish-orange color, suggesting a potentially older stellar population. This secondary component appears tidally distorted, likely gravitationally influenced by the primary component. The overall system displays tidal features, indicative of ongoing gravitational interactions and dynamical disruption. A substantial fraction of the system’s light is concentrated in the brighter, central region, indicating a dense stellar population and active galactic nucleus presence. The morphology suggests a system with moderate stellar mass and a suppressed star formation rate relative to its mass.
