The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a central concentration of light, with a gradual decrease in intensity towards the outer regions. The overall color is slightly reddish, suggesting an older stellar population, although there are hints of bluer regions as well. The galaxy's shape is somewhat elongated, but not dramatically so. There is no clear evidence of spiral arms or significant dust lanes. The structure appears largely undisturbed, showing no major signs of interaction or recent merging activity.
