The galaxy appears to be an elliptical galaxy, possessing a relatively smooth and featureless morphology. Its light profile is centrally concentrated, exhibiting a radial gradient of decreasing brightness outward. The shape is largely round, with a slight deviation from perfect circularity. The color appears to be somewhat redder, suggesting an older stellar population. There are no prominent spiral arms, bars, or dust lanes visible. No major mergers are visually evident, with a smooth distribution of light indicating the potential for little to no recent disturbances. The overall appearance indicates a passively evolving galaxy.
