The galaxy presents as a relatively smooth, elliptical structure. Its core appears intensely bright, suggesting a high concentration of stars or an active galactic nucleus, though the image resolution limits further discrimination. There are hints of a slight elongation, deviating from a perfect circularity. The color profile indicates an older stellar population. Given the overall morphology, a low rate of star formation is implied. Evidence shows no significant signs of ongoing mergers or major disturbances in the galaxy's structure. A slight hint of a disk structure can be noticed.
