The galaxy presents as a disturbed system, potentially undergoing a merger event or recent interaction. Morphologically, the galaxy lacks a clear spiral arm structure or a well-defined elliptical shape. Instead, the overall form is irregular and elongated. The central region shows a higher concentration of luminosity, suggesting a core or nucleus. The light profile appears relatively smooth, however, there is a noticeable asymmetry and disturbance in the outer regions. Patches or streams of stellar material deviate from the main body, indicating tidal forces at play. The color gradient suggests a population of young, blue stars, particularly in the regions of disruption. Based on the color profile it looks like there are some areas of older, redder stars mixed in with some degree. Overall, there is clear evidence of an ongoing or recent interaction, suggesting the system is not in equilibrium.
