The galaxy presents as a relatively smooth, elliptical structure. Its core appears to be a bright, concentrated spheroid. The galaxy exhibits a yellow-white hue, possibly indicative of an older stellar population. There is a slight elongation in its shape, leaning toward a cigar-like form. There is no distinct dust lane apparent. The outer regions of the galaxy gradually fade into the background sky, suggesting a diffuse stellar halo. Overall, it appears to be a mature, quiescent galaxy with no strong signs of recent mergers or significant star formation activity.
