The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central bulge that appears more concentrated and features a yellow-ish hue, suggestive of an older stellar population. The outer regions of the galaxy are less defined, gradually fading into the background. The color of the outer regions trends towards blue, potentially indicative of some degree of ongoing, or more recent star formation, albeit at a low rate. Overall, the galaxy displays a gently elongated shape without any obvious signs of significant tidal disturbances or ongoing merger activity.
