The galaxy appears to be undergoing a significant merger event. The primary galactic component presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears fairly even and its colour is yellowish, suggesting an older stellar population.

There is a clearly defined secondary component, visually separated from the primary galaxy. This secondary component displays a distinctly redder hue, potentially indicating a region of intense star formation or a higher dust content. The morphology of this component is less defined, appearing somewhat irregular and elongated, possibly due to tidal interactions with the main galaxy.

The overall impression is one of a dynamic system, actively reshaping itself through gravitational interaction.
