The galaxy presents as a relatively smooth, elliptical-like structure. The central region appears more concentrated, exhibiting a yellowish-white hue, possibly indicative of an older stellar population. Moving outwards from the center, the color transitions to a bluish-white, with a less concentrated distribution. This potentially signifies younger stars or lower metallicity gas and dust in the outer regions. Overall, the galaxy shows a lack of prominent spiral arms or distinct features, and it has a fairly regular shape, without signs of major mergers or interactions.
