The observed galaxy presents a morphology indicative of an ongoing or recent merger event. Its overall shape is significantly distorted, lacking a clear spiral or elliptical structure. A prominent, bright core region is observed, exhibiting a bluish hue. This suggests a population of hot, young stars within the core, possibly triggered by the merger event.

Extending from the core is an elongated structure appearing reddish-orange. This could be a tidal tail composed of older stars and dust, or a remnant of the original disk. The light intensity diminishes towards the end of the tail, suggesting that the stellar population is less dense or that dust obscuration is more significant.

The galaxy exhibits complex features suggesting significant gravitational interactions. A secondary, less prominent concentration of light is seen in the vicinity of the main body, which could be a smaller galaxy interacting with the larger one. The galaxy's overall appearance indicates it is in a dynamically active state.
