The galaxy presents a primarily smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge, suggesting a high stellar density in its core. The color is predominantly yellowish-orange, possibly indicating an older stellar population with diminished recent star formation. Subtle, asymmetrical features suggest minor gravitational disturbances, perhaps related to a recent small merger event. The light distribution is not perfectly symmetrical, and shows signs of interactions or the accretion of smaller galaxies. A central core of concentrated light and mass is well defined.
