The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The system appears to be composed of two distinct components: a primary, more concentrated central region, and an elongated tidal tail extending from one side. The central region displays a yellowish-orange hue, suggesting a population of older stars, while the tail shows a similar color. The overall shape of the galaxy is highly irregular, lacking a defined spiral or elliptical structure. This distortion points towards gravitational interactions disrupting the galaxy's original form. The presence of a tidal tail further supports this hypothesis, representing material stripped away during a merger or close encounter with another galaxy. The system seems to exhibit intermediate star formation activity.
