The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that appears yellow, suggesting an older stellar population dominating the core. The galaxy's overall shape is neither perfectly round nor strongly elongated, leaning more towards a somewhat flattened spheroid. There is no clear evidence of spiral arms or significant dust lanes visible in this image. The outer regions show a gradual fading in luminosity, suggesting a declining density of stars at larger radii. There are no apparent signs of major ongoing mergers or significant tidal disturbances.
