The galaxy presents as an elliptical, relatively smooth structure with a noticeable central bulge. The core is intensely luminous, transitioning smoothly to a less bright outer region. The shape deviates slightly from a perfect circle, exhibiting a hint of elongation. There is little evidence of spiral arm structure or significant dust lanes. The color gradient suggests a population of older stars, and the overall morphology indicates a relatively evolved system. The apparent lack of strong blue emission suggests low current star formation activity, but the luminosity implies it is still a very massive galaxy. There is no indication of ongoing major mergers, but there may be some signs of minor interaction.
