The galaxy exhibits a disturbed morphology suggestive of an ongoing or recent merger event. Two distinct luminous regions are visible. One is bluer in color, indicating a higher concentration of younger, hotter stars. The second region appears more yellow/red, suggesting an older stellar population. The galaxy lacks a clear, defined spiral structure or a well-defined elliptical shape. A faint, extended halo or tidal feature appears to surround the main body, indicating gravitational interaction with another galaxy. Dust lanes or significant obscuration are not readily apparent. The overall structure appears irregular and complex. There is evidence of a significant merger occuring.
