The galaxy presents an irregular morphology, likely indicative of an ongoing or recent merger event. There are at least two distinct luminous components, suggesting the presence of separate galactic nuclei or dense stellar clumps. The color distribution appears uneven, with a region exhibiting a bluer hue, possibly indicative of ongoing star formation. The overall light distribution is relatively smooth, but there is a degree of disturbance, with the overall appearance suggesting a dynamically active system.
