The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There's a general lack of distinct features such as spiral arms or a prominent disk. The light is dominated by yellow to orange hues in the core, suggesting an older stellar population. There is a slight elongation visible, deviating from a perfectly circular shape. The outer regions display fainter and bluer tones. There is no evidence of a major ongoing merger event, although some minor disturbances cannot be ruled out. The overall impression is of an evolved system, possibly an elliptical galaxy, with low current star formation activity.
