The galaxy presents a complex morphology, appearing to be undergoing an interaction or merger event. There is a dominant, relatively smooth component of light with a roundish appearance. However, there is a distinct, elongated feature extending from this central region. This extension exhibits a more irregular, disturbed structure and shows bluer colours compared to the main body. The overall colour gradient suggests a population of younger, star-forming regions within the disturbed feature, while the smoother component is likely composed of an older stellar population. There is some evidence of tidal tails or debris around the galaxy, hinting at gravitational interactions with other galaxies. Based on these observations, it appears that this is a galaxy with a high likelihood of recent or ongoing merger activity, leading to enhanced star formation in the region.
