The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. The galaxy appears to be generally spheroid, with no discernible spiral arm structures or a distinct galactic disk. The light distribution within the galaxy suggests a dominant old stellar population. The core region appears nearly uniform in color, trending towards yellow. The outer edges show some signs of color variation, potentially from younger stars. There may be minor disturbances in the galaxy's structure which could be indicative of past or ongoing interactions with other galaxies, however no obvious merging companion is observed. No significant dust lanes or regions of intense star formation are visible. The galaxy is relatively compact, suggesting a moderate physical size and a reasonably high stellar density.
