The galaxy exhibits a relatively smooth morphology. The light profile suggests a high degree of central concentration. The galaxy appears to have two distinct central cores or is possibly undergoing a merging event. The dominant core is more intense and has an orange hue, which likely indicates an older stellar population. A less luminous object can be seen next to the more luminous body of the object, though whether it is part of the object or a result of gravitational lensing is difficult to discern. No spiral arms or clear disk-like structure are visible. The overall shape can be described as nearly circular, although there is a slight deviation from perfect roundness. The color gradient suggests that star formation is relatively low or has ceased in the core. The outer regions have a slightly bluer tint than the core. This may point to ongoing star formation in the outer regions.
