The galaxy presents as a somewhat elongated, elliptical structure with a smooth, diffuse appearance. The central region exhibits a higher concentration of light, appearing brighter and with a yellowish hue, suggesting an older stellar population. Moving outwards, the light gradually fades, with subtle color variations towards the edge. There is a hint of bluer tones in the surrounding region, implying the potential presence of younger stars or ongoing star formation. The overall morphology indicates a system that is not undergoing significant interaction or disturbance, showing a relatively quiescent state. The shape can be described as somewhere between round and cigar-shaped, with no clear signs of spiral arms or a defined disk component.
