This galaxy exhibits a generally smooth morphology with a bright, concentrated central region. The light is fairly uniform and decreases gradually outward from the center, suggesting a relatively old stellar population. There's a subtle bluer hue in the inner regions, hinting at some ongoing, but limited, star formation within the galaxy's core. The galaxy is largely elliptical in shape, appearing quite round with only minor deviations from perfect circularity. There are no readily apparent signs of spiral arms or other significant features, though there is some evidence of minor disturbances in the outer regions. Overall, the galaxy seems to be a fairly isolated system, showing no strong indications of recent or ongoing mergers.
