The galaxy appears elliptical in shape, exhibiting a smooth, concentrated central bulge that diminishes outwards. The color profile suggests an older stellar population, as evidenced by the dominant yellowish-orange hue in the core. Fainter blueish arms can be seen extending from the centre of the galaxy. There's no indication of major ongoing star formation or significant dust lanes. The galaxy presents a degree of roundness. No signs of tidal disturbances, major mergers, or prominent active galactic nuclei features are apparent. The overall light distribution and morphology point towards a galaxy likely located at a non-negligible cosmological distance, yet still exhibiting sufficiently resolved features.
