The galaxy presents as a morphologically complex system, possibly undergoing a merger event. There are two distinct, luminous components. The larger component exhibits a smoother, more diffuse appearance, with a color gradient shifting from a yellow core to a bluer outer region. The second component is smaller, more compact, and displays a distinctly redder hue. There are subtle indications of tidal features or disturbances, such as faint extensions or asymmetries in the outer regions, suggesting gravitational interactions. The overall shape is not clearly defined, but the system is neither perfectly elliptical nor clearly disk-shaped. The color suggests the presence of both older stellar populations and regions of ongoing or recent star formation.
