The galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy, with a notable lack of distinct spiral arms or a central bar. The light distribution is fairly concentrated toward the core, suggesting an older stellar population may dominate. The galaxy appears largely undisturbed, without significant signs of mergers or tidal interactions. There might be some evidence of low-level star formation in the outer regions, potentially giving it a slightly bluer color gradient moving outward.
