The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its color gradient suggests a population of older stars, exhibiting a yellowish-red hue indicative of evolved stellar populations. There is no apparent dust lane or significant spiral arm structure. The galaxy appears somewhat round and undisturbed, with little evidence of recent major merger activity. There might be slight indications of a minor disturbance. The overall morphology suggests a transition towards a more passive state of star formation.
