The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated luminosity. There is a suggestion of a slight elongation in the morphology. The core region appears brighter and more yellow in color. The outer regions exhibit a gradual decrease in luminosity and a subtle shift toward a slightly redder hue. No distinct spiral arms or prominent dust lanes are discernible from the image, and there is little indication of any ongoing major merger activity or significant morphological disturbance. The overall appearance suggests a galaxy dominated by an older stellar population.
