The galaxy presents a primarily smooth, elliptical morphology. It exhibits a central bulge that is relatively indistinct from the surrounding halo, lacking prominent features such as spiral arms or a distinct disk. The galaxy appears to have a slightly elongated shape, deviating from a perfectly circular form. There are no obvious signs of ongoing major mergers, however there is a slight chance for minor disturbances. The galaxy's light profile appears concentrated towards the center, gradually fading towards the edges. The overall color of the galaxy suggests an older stellar population, consistent with a lower rate of star formation.
