The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable color gradient, transitioning from a yellow-orange core to a slightly greener outer region, suggesting potential variations in stellar population or dust distribution. The galaxy exhibits a high degree of symmetry, indicating a relaxed state and minimal signs of recent major mergers or tidal disturbances. There is little evidence of prominent spiral arms or significant star-forming regions. The overall morphology suggests a more evolved galaxy, possibly with a dominant population of older stars and a relatively low rate of star formation. The galaxy is approximately circular, with a very slight elongation. 
