The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a high concentration of light, appearing a warm orange hue, suggesting an older stellar population. The light gradually diffuses outward, fading into the darker background. While appearing mostly homogenous, there's a subtle elongation visible, with the galaxy extending slightly more along one axis than the other. There is no clear spiral arm structure or evidence of significant dust lanes apparent in this image. The outer regions appear diffuse and indistinct, lacking sharp boundaries. The overall impression is of a galaxy that is not actively undergoing significant star formation.
