The galaxy exhibits a morphology indicative of an ongoing or recent merger event. There are two distinct concentrations of light, a brighter, more diffuse region and a slightly smaller, more concentrated region, suggesting either two galactic nuclei or a nucleus and a region of intense star formation triggered by the interaction. The overall shape of the galaxy is irregular, lacking a well-defined spiral or elliptical structure. There is a hint of tidal features or faint extensions of light emanating from the main body, further supporting the merger hypothesis. The color gradient across the galaxy is noticeable, with the brighter region appearing bluer, possibly indicating a younger stellar population and ongoing star formation. The less bright region exhibits a more reddish-orange hue, which could signify an older stellar population. The galaxy appears relatively bright, suggesting a significant amount of star formation.
