This galaxy exhibits characteristics of a system undergoing a significant merger. The primary body of the galaxy presents a relatively smooth, albeit somewhat disturbed, morphology. There are noticeable tidal features suggesting ongoing gravitational interaction and disruption. A secondary concentration of light is visible, appearing connected to the main galaxy via a faint bridge of material. This suggests that the "secondary concentration of light" is an actively merging companion galaxy.

The color distribution indicates a mix of stellar populations. The central region appears more yellow/white, consistent with older, more evolved stars. The outer regions, including some of the tidal features, display a bluer hue, suggestive of younger, hotter stars and recent or ongoing star formation. The overall shape is irregular, lacking a well-defined disk or spiral structure, further supporting the conclusion of an ongoing merger.
