The galaxy presents as a moderately luminous, yellowish-orange, elliptical-type galaxy. It appears to be relatively smooth in texture, with a centrally concentrated light profile. There is a slight elongation visible, suggesting it is not perfectly spherical. No distinct spiral arms or bar structures are apparent. There's no significant dust lane observed. The galaxy shows a well-defined core and gradual decrease in light intensity from the center outward. The color indicates an older stellar population. There is no evidence of recent major merger activity, though slight asymmetry suggests a minor interaction cannot be ruled out.
