The galaxy appears as a centrally concentrated object with a largely smooth morphology. The light profile indicates a significant bulge component. The color is generally consistent, with the inner regions appearing more yellow/orange than the outer regions which are green/blue. There is no clearly visible disk structure, and there appear to be no signs of significant ongoing mergers or major tidal disturbances, although a very slight asymmetry in the outer regions could suggest minor interactions or disturbances. The overall shape is relatively circular. Given its moderate redshift, the galaxy is likely a massive system exhibiting ongoing star formation at a relatively high rate.
