The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, lacking any discernible spiral arm structure or prominent disk features. The light distribution suggests a single spheroidal component with no signs of significant bars, rings, or tidal tails. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating the central regions, or a dusty core. The outer regions fade in intensity with a somewhat bluer tone, possibly indicating the presence of younger stars within the extended halo, or that the older population of stars is heavily obscured. The galaxy does not show any signs of ongoing major merger activity or significant morphological disturbances, appearing largely undisturbed. There may be signs of a minor disturbance, but this could also be due to noise from the imaging.
