The galaxy presents as a largely featureless, elliptical or spheroidal structure with a smooth, concentrated light profile. Its color gradient suggests a centrally concentrated population of older stars, inferred from the yellowish-orange hue at the core, gradually fading into a redder halo. There is no obvious sign of spiral arms or significant dust lanes. No disturbances are visibly present, and there is no evidence of tidal tails or ongoing mergers.
