The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is bright and yellow-orange in color. This coloration may indicate an older stellar population within the bulge. Moving outward from the center, the light gradually fades and becomes less saturated. There is a slight indication of a faint disk, which is oriented horizontally in the image frame. The outer regions appear more diffuse and blueish, possibly indicating ongoing, but low-level, star formation in these regions, or a younger stellar population. There is no obvious presence of spiral arms or significant dust lanes and no evidence of any other galaxy mergers. The galaxy is slightly elongated and is not perfectly circular.
