The galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge that fades gradually into a diffuse halo. The light distribution appears largely uniform, suggesting a well-mixed stellar population with a lack of prominent star-forming regions or distinct spiral arm structures. There is a slight blue tinge to the outer portions of the galaxy, suggesting some lower-level star formation. The galaxy appears largely undisturbed, without clear signs of recent mergers or significant tidal interactions with neighboring galaxies. The system demonstrates high rotational symmetry.
