The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a bright, slightly blue core that diffuses outward. This likely indicates a significant population of older stars dominating the overall light output, with a degree of recent star formation.

There is a faint hint of an extended halo surrounding the central region, though the resolution makes it difficult to discern any distinct features such as spiral arms or dust lanes. The overall color appears relatively uniform across the galaxy, suggesting a well-mixed stellar population and a lack of significant dust obscuration. The galaxy does not appear to be undergoing any major mergers or tidal disruptions, it looks relatively undisturbed.
