The galaxy presents as a system undergoing a significant merger event. A primary, relatively smooth, elliptical-like component dominates the structure. This central region exhibits a yellow-orange hue, suggestive of an older stellar population, possibly with minimal current star formation.

Extending from the main body, there appears to be a tidal tail or bridge of material. This feature appears reddish-orange in color. It's length is is approximately comparable to the central body's width, indicating a notable interaction.

Another, more irregular component is visible on the opposite side of the primary galaxy. This feature exhibits clumpy morphology and a somewhat bluer tint, possibly indicating younger stars or ongoing star formation activity, although it also may represent a region affected by tidal forces.

The overall system appears disturbed, lacking a well-defined disk or spiral structure. The significant tidal tail and disturbed morphology suggests a recent and ongoing merger event with another galaxy of notable size. Based on the color indices, the system appears to be a relatively massive galaxy with a suppressed star formation rate, currently experiencing a merger.
