The galaxy presents as an elliptical type, exhibiting a generally smooth morphology with a high degree of central concentration. The primary body of the galaxy is predominantly yellow, suggesting an older stellar population dominating the light output, though it is possible there is significant dust reddening the galaxy. There is a slight color gradient, with a concentration of bluer emissions towards the left side of the galaxy, which may indicate ongoing or recent star formation in a concentrated region. The galaxy displays a moderate degree of roundness. There is no obvious indication of a spiral arm structure. There are no apparent signs of major mergers or significant tidal disturbances, though a slight asymmetry could suggest minor gravitational interactions. 
