The galaxy appears to be part of an interacting system consisting of two distinct components. Both components exhibit a blue hue, suggesting the presence of relatively young, hot stars, indicative of ongoing or recent star formation. The brighter component displays a more compact, centrally concentrated morphology, possibly a bulge or a region of intense star formation activity. The second component, while still showing a relatively compact size, appears somewhat more diffuse. There is a noticeable connection between these components, suggesting tidal interaction. The structure of the galaxy system overall seems irregular, indicating a disturbance to the morphology, possibly caused by gravitational interactions. The system does not appear to have a smooth elliptical profile, but rather a more complex and disrupted structure.
