The galaxy presents as a smooth, elliptical-like structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue. This suggests a population of older stars dominating the galactic center, with potentially less active star formation occurring in that region. 

Moving outwards from the core, the color shifts towards a more reddish tone. This might indicate the presence of an older stellar population and some dust absorption in the outer regions of the galaxy. A slight asymmetry is visible on one side, hinting at possible gravitational interaction or tidal disturbance. The galaxy appears elongated, approximately twice as long as it is wide, with a flattened shape.
