This galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology with a high degree of roundness, showing only minor deviations from a perfect circular shape. The color profile reveals a redder core, suggesting an older stellar population dominating the central region. The outer regions display a bluer hue, hinting at the presence of younger stars, although these are not distinctly resolved. There is a slight asymmetry or minor disturbance in the disk, possibly indicating a past or ongoing minor interaction or merger event. The galaxy does not exhibit any obvious spiral arm structure, indicating that this galaxy is likely a quiescent galaxy.
