The galaxy appears to be composed of multiple interacting components. A central, elongated structure dominates the view, displaying a smooth, featureless morphology. This core component exhibits a yellowish-white hue.

To the left of this main body, a smaller, more rounded component is visible. It shares a similar yellowish-white coloration, indicating a similar stellar population or dust content. There is evidence of potential tidal interaction between these two components, hinting at an ongoing or recent merger event.

On the far right, a distinct, compact red structure is visible. This may be a region of intense star formation activity. Given the interactions apparent in the system, such activity may be triggered by the disturbance.

The overall morphology suggests a system in transition, possibly evolving from a spiral or irregular galaxy into a more elliptical or peculiar form due to the merger. Further spectral analysis is required to precisely determine the nature of the red structure and the stellar populations present within the different components of the galaxy.
