The galaxy presents as a single, relatively smooth, centralized light source. It appears largely spheroidal in shape, with a high degree of central concentration. There is a slight color gradient with a subtle bluish tint around the outer edges, transitioning towards redder hues closer to the central core, suggestive of varying stellar populations. The overall structure does not indicate any significant tidal disturbances, spiral arms, or other complex morphologies. Light output suggests intermediate star formation activity and a considerable stellar mass. There are no obvious indications of a recent major merger. The primary classification would likely be an elliptical galaxy.
