The galaxy presents as a fairly smooth and rounded structure. The central region exhibits a concentrated, bright core, indicative of a significant stellar population or potentially an active galactic nucleus. The color gradient transitions from a yellowish core outwards to a slightly bluer halo. There is no evidence of a prominent disk or spiral arm structures; however, the faint blue periphery suggests the presence of some ongoing star formation. Overall, the galaxy morphology points towards an elliptical type. There is no clear evidence of major ongoing mergers or significant tidal disturbances. The object appears relatively isolated and undisturbed.
