The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology is primarily elliptical, exhibiting a gradual fading in luminosity from the core outwards. The central region is notably brighter and more yellow in color, suggesting an older stellar population dominating in the galactic nucleus. A disk is not readily discernible, and there are no obvious spiral arm structures. There may be some subtle features indicating minor disturbances in the outer regions, but no major merging events are apparent. Overall, the galaxy presents as a relatively evolved system with a significant spheroidal component.
