The galaxy appears as a faint, elongated object. There is a subtle reddish hue, suggesting it may be a relatively old galaxy with a population of redder stars or significant dust obscuration. Based on its shape, there is possible evidence of disruption. It is difficult to classify the galaxy as either elliptical or spiral. The galaxy is a potential merger with a larger and smaller component. There is also an unusual amount of noise that seems to be coming from the galaxy. The galaxy is relatively compact. Further investigation will be needed to fully understand the nature of this galaxy.
