The galaxy presents as two distinct structures. The larger component appears as a relatively smooth, rounded object with a cyan hue. The smaller component is elongated and displays a gradient in color, shifting from yellow to a lighter shade. The overall morphology suggests a possible ongoing interaction or merging event between these two components. The more rounded, cyan-colored component exhibits a smooth distribution of light. The elongated component appears more disturbed or asymmetric, with a hint of structure. The color differences between the two components suggest varying stellar populations or dust content, with the cyan suggesting the presence of younger, hotter stars within the larger component. The elongation of the smaller component implies a more elliptical shape. There are no apparent spiral arms, but the resolution of the image is low. The system's apparent interaction suggests it is a dynamic object experiencing gravitational forces and likely elevated star formation activity.