This galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution is dominated by a yellowish-white hue, suggesting a stellar population primarily composed of older stars. The overall shape is moderately elliptical, appearing more in-between circular and elongated. There is no clear evidence of spiral arms, prominent dust lanes, or a distinct galactic disk. Minimal structural disturbances are visible, suggesting no recent major merger events. The galaxy seems to be relatively isolated and undisturbed. The object shows characteristics consistent with a quiescent elliptical galaxy.
