The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing nearly round in shape with a slight suggestion of elongation. The core region displays a bright, diffuse glow that diminishes gradually outwards. The observed color profile suggests a population of older stars dominating the light output, giving it a reddish-yellow hue with subtle blue-green tinges closer to the center. There is no apparent spiral arm structure or significant dust lane obscuration discernible within the optical data. There are no readily visible signs of a recent major merger event; it may be undergoing only minor disturbances. The galaxy's apparent size on the sky is small, indicating a moderate physical scale at its redshift distance.
