The galaxy presents an overall elliptical morphology, appearing largely smooth in texture with no readily apparent spiral arm structures. The central region exhibits a brighter, concentrated core, suggesting a significant stellar density. A slight flattening is observed, deviating from a perfectly circular shape. The color distribution indicates a gradient, with a bluer hue dominating the outer regions, potentially indicative of ongoing star formation, while the core shows a redder tint, possibly due to an older stellar population. Evidence of possible minor tidal disturbance is seen at one end of the galaxy in the form of a slight extension of the surrounding halo. There's a slight asymmetry, with one side of the galaxy appearing somewhat more extended than the other. The lack of significant dust lanes or distinct features supports its classification as a relatively undisturbed system.
