The galaxy presents as a generally smooth, centrally concentrated object. It is a roughly elliptical shape with a high degree of symmetry. The core exhibits a bright, yellowish hue that fades into a less intense, redder outer region. There is little indication of spiral arms or distinct features within the galaxy's morphology. No signs of ongoing major mergers or tidal disturbances are immediately evident. The overall light distribution suggests a more evolved stellar population, potentially characteristic of an elliptical galaxy.
