This galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a concentrated spheroid shape with minimal discernible internal structure. Its color is predominantly yellow, suggesting an older stellar population with diminished ongoing star formation. There is a slight hint of blue in the outer regions, potentially indicating pockets of younger, hotter stars, or possibly artifacts. The galaxy's shape deviates from a perfect circle, showing a slight elongation. The faintness of the galaxy indicates that the light is coming from a significant distance from the Earth. Finally, there is a distinct, slightly more compact secondary core to the galaxy, perhaps evidence of a prior merger.
