The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high degree of luminosity, indicative of a concentrated stellar population or possible active galactic nucleus. Moving outwards from the core, the light profile gradually diminishes, with the isophotes appearing moderately elliptical. There is a slight asymmetry in the distribution of the outer regions, with one side appearing subtly more extended than the other. Overall, the galaxy lacks any prominent spiral arm structures or significant dust lanes. Its color appears somewhat redder, which may indicate a population of older stars, potentially suggesting that star formation has slowed down. The general morphology suggests it is a fairly well-evolved system.
