The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge with a moderate degree of ellipticity, appearing elongated in shape. The color gradient suggests a central region that is redder in comparison to the surrounding areas, possibly indicating an older stellar population dominating the core. A fainter, blueish-green halo surrounds the central bulge, which may indicate some ongoing, though likely subdued, star formation. No significant signs of mergers or tidal disturbances are readily apparent.
