The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. Moving outwards from the core, the light gradually fades, transitioning to a more reddish-yellow colour, suggesting a change in stellar population and/or dust content. The shape is somewhat elliptical, but appears mostly round. There is no apparent spiral structure or distinct features such as star-forming regions or dust lanes visible in this image, suggesting a relatively quiescent and evolved system. There is a hint of a surrounding halo, but its intensity is very faint compared to the main body of the galaxy. No significant signs of tidal disturbances or ongoing mergers are apparent.
