The galaxy presents as a singular, well-defined object with a smooth, elliptical morphology. It exhibits a high degree of central concentration, with the luminosity appearing to peak strongly towards the core. The outer regions of the galaxy fade gradually, with no discernible spiral arms or significant features such as dust lanes or prominent star-forming regions visible in this image. The overall color of the galaxy appears to be slightly reddish, suggesting an older stellar population and a relatively low rate of on-going star formation. There is no evidence of any ongoing major merger activity or significant tidal distortions. The galaxy appears isolated and undisturbed within its immediate vicinity.
