The galaxy presents as a somewhat elliptical structure with a high degree of central concentration. The light distribution suggests a relatively smooth morphology, lacking prominent spiral arms or distinct features. The core region exhibits a yellow-orange hue, which could indicate an older stellar population and/or significant dust obscuration. Moving outward from the center, the color shifts subtly towards redder tones. There is some slight indication of disruption to the structure of the galaxy, perhaps interaction with another galaxy.
