The galaxy presents as an elliptical system, exhibiting a smooth, centralized light profile with no discernible spiral arm structure. It appears moderately luminous, with a concentrated core that gradually fades towards its outer regions. The galaxy's shape is generally oblate, deviating slightly from a perfect circle, but not exhibiting extreme elongation. There is no indication of major merger activity, although some minor disturbances cannot be ruled out at this resolution. Color gradients suggest the presence of an older stellar population. It displays a yellow hue centrally with slightly redder tones in the outer halo. Star formation is likely suppressed, as evidenced by the lack of blue light indicative of young, hot stars. The galaxy appears isolated, lacking any close companion galaxies which could induce tidal interactions.
