The galaxy presents as a relatively smooth, elliptical object. The light is concentrated in the center, with a yellowish-white hue indicative of an older stellar population. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy appears largely undisturbed, with no obvious signs of recent major merger events. It exhibits a fairly rounded morphology. Marginal irregularity is visible in the outskirts, possibly indicative of tidal interactions or minor disturbances.
