The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is primarily elliptical, appearing somewhat rounded, with a slight deviation from perfect circularity. There is little to no evidence of spiral arm structure or a well-defined disk. The galaxy exhibits a general yellow-white hue, suggestive of an older stellar population and potentially lower levels of current star formation. No obvious signs of major mergers or significant tidal disturbances are apparent. The galaxy's overall structure indicates a gravitationally relaxed system that is relatively evolved.
