The galaxy presents as a centrally concentrated, relatively smooth object. The light profile appears to be dominated by an elliptical component with a high degree of roundness. There is little evidence of spiral arm structure or significant dust lanes. Color gradients suggest a possible variation in stellar populations or dust content, with a somewhat bluer hue towards the outer regions. The overall light distribution indicates a galaxy that is likely well-evolved, with ongoing low levels of star formation. There does not appear to be any major disturbances or signs of ongoing merging activity.
