The galaxy presents as a centrally concentrated, smooth elliptical object. It exhibits a subtle color gradient, transitioning from a relatively redder core to slightly bluer outer regions. The central bulge appears well-defined and dominates the galaxy's light profile. No distinct spiral arms or significant dust lanes are discernible. The overall morphology suggests a lack of ongoing major star formation within the galaxy, and likely a high fraction of older stars in the bulge. There's a subtle asymmetry in the outer isophotes, possibly indicating a minor gravitational interaction or disturbance, though the smooth texture otherwise suggests a relaxed structure. The shape appears very close to circular.
