The galaxy presents as a relatively smooth, elliptical form. There is a concentrated central bulge exhibiting a yellowish-orange hue, indicative of an older stellar population. The outer regions appear less concentrated and exhibit a faint greenish-blue color gradient, potentially suggesting the presence of some younger stars or ongoing, albeit low, star formation activity in the outer disk or halo. The overall structure appears largely undisturbed, with no obvious signs of recent major merger activity, although a subtle asymmetry or minor disturbance cannot be entirely ruled out. The galaxy is significantly flattened but not so much that it would be considered a spiral galaxy.
