The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The overall color suggests an older stellar population, with a yellowish-orange hue dominating the core region. The light distribution is centrally concentrated, fading gradually towards the outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a generally round shape, with a high degree of rotational symmetry. No signs of any major mergers or tidal disturbances are apparent, suggesting a relatively undisturbed evolutionary history. There is some evidence of light that extends beyond the main body of the galaxy, but it is faint and smoothly distributed, possibly indicating a stellar halo.
