This galaxy appears to be undergoing a significant interaction or merger. The morphology suggests a complex system with multiple distinct luminous components.

One component displays a relatively smooth, round appearance with a bright, concentrated core, exhibiting a blue-white color indicative of younger stellar populations. Adjacent to this, there are at least two other discernible components, both exhibiting a yellower hue, possibly representing regions of older stars or dust obscuration. These appear less centrally concentrated and somewhat more diffuse.

The overall shape is irregular and distorted, lacking a clear spiral or elliptical structure. This disruption could arise from gravitational interactions or a merger event. Faint tidal features or extended diffuse light might be present but are difficult to discern with certainty at this resolution. The presence of multiple nuclei and distorted morphology supports the possibility of an ongoing merger.
