The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The core exhibits a yellowish-orange hue, suggesting an older stellar population and a lack of significant ongoing star formation. The isophotes appear generally round, with a slight deviation towards an in-between shape. There's a faint, diffuse halo surrounding the central bulge, extending outwards. No strong spiral arm structure or prominent dust lanes are discernible in this image. The overall morphology indicates a system that is not undergoing any major or minor mergers. A possible minor disturbance on the edge may be present.
