The observed galaxy presents a generally smooth morphology. It exhibits a nearly round shape with some deviation from perfect circularity. There is evidence of a potential interaction or merger event. A secondary, more compact object appears in close proximity to the primary galaxy. It is unclear whether this is tidal debris, a satellite galaxy, or another merging galaxy.

The primary galaxy displays a color gradient, appearing bluer in its outer regions and redder towards its core. The redder central region could indicate an older stellar population or higher dust content.
