The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The color index suggests a redder population, indicative of an older stellar population and a lower rate of on-going star formation. There is a slight elongation, however the object looks largely round. 
