The galaxy presents a somewhat diffuse, elliptical morphology. There is a central concentration of light that appears slightly brighter than the outer regions. The color profile suggests a population of older stars, indicated by the reddish-orange hues throughout the galaxy. There's minimal evidence of significant dust lanes or spiral arm structures, which supports its classification as a galaxy on the smoother end of the morphological spectrum. I note some disturbances in the galaxy's apparent shape and color that suggest there may be a minor merger occurring, although the galaxy appears relatively undisturbed overall.
