The galaxy presents a generally smooth morphology, with a high probability of being smooth rather than exhibiting prominent features or a disk structure. Its shape appears intermediate in roundness, leaning toward elliptical but not perfectly circular. There is no significant evidence of major mergers or strong tidal disturbances in this image, but minor disturbances cannot be ruled out. The galaxy exhibits a redder color in its central region, suggesting an older stellar population, with bluer hues in the outer edges, hinting at more recent star formation, albeit at a low rate. The estimated stellar mass indicates it is a relatively massive galaxy.
