The galaxy presents as a somewhat elliptical structure, elongated along a preferential axis. Its overall appearance is smooth, without readily discernible spiral arms or dust lanes. A bright central bulge is apparent, gradually fading into the outer regions of the galaxy. The color profile suggests a population of older stars, giving it a yellowish hue, although the suggestion of some bluer star forming regions cannot be discounted. There is no obvious indication of strong tidal interactions or major mergers with other galaxies, although there is a hint of a minor asymmetrical structure in the outer disk, which could point to a minor merger or disturbance. Overall, the galaxy seems relatively undisturbed and evolved.
