The galaxy presents as a primarily smooth object with a high degree of central concentration. There is a notable absence of distinct spiral arms or a well-defined disk structure. The galaxy appears roughly circular in shape. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Fainter greenish color is observable surrounding the nucleus, possibly indicating a younger stellar population or some ongoing star formation, but the overall color profile suggests a evolved stellar population dominating the light output. Overall, the galaxy appears to be in a relatively quiescent state, with no prominent signs of active galactic nuclei activity or major ongoing mergers. There may be minor disturbances or an interaction affecting the outer halo.
