The galaxy exhibits a notable asymmetry, appearing to be composed of two distinct, interacting components. The larger, primary component displays a yellowish hue, suggesting an older stellar population and potentially lower levels of active star formation. Its overall structure appears relatively smooth. The secondary component, located in close proximity to the primary galaxy, is smaller and exhibits a bluer color, indicative of a younger, hotter stellar population and ongoing star formation. There is some distortion in the shape, suggesting potential tidal interaction or a merger in progress. A faint bridge of light appears to connect the two components. The morphology suggests a system undergoing a minor disturbance, potentially a tidal interaction or a minor merger event.
