The galaxy presents as a relatively smooth, elliptical structure. There is a noticeable concentration of light towards the center, indicative of a central bulge. The galaxy exhibits a yellowish-white color, suggesting a population of older stars. Although it appears mostly undisturbed, there are subtle irregularities in its shape, implying the possibility of minor gravitational interactions or past merger events. These disturbances manifest as slight asymmetry. There are no readily apparent spiral arms or significant dust lanes. The outer regions of the galaxy appear fainter, fading gradually into the background sky.
