The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, mostly featureless morphology. It displays a high degree of central concentration with a bright core. The overall shape is approximately circular. There is a distinct color gradient, transitioning from a yellowish-white core to a redder outer halo. No spiral arms or significant dust lanes are discernible. The light distribution suggests an older stellar population dominating the galaxy's composition, with low ongoing star formation. There is no evidence of any major interactions or mergers in its recent history, although minor disturbances cannot be ruled out.
