The galaxy presents as a centrally concentrated object, exhibiting a morphology consistent with an elliptical galaxy. It displays a smooth luminosity profile, with the highest surface brightness located at the galactic center. The isophotes appear elongated, suggesting a moderate degree of ellipticity. There is no obvious spiral arm structure or dust lane. There is a color gradient, with the central regions appearing more yellow/white, potentially indicating an older stellar population, while the outer regions have a subtle bluish tinge. The overall appearance suggests a relatively evolved system with ongoing, but likely subdued, star formation activity in the outer reaches.
