The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light profile with minimal discernible substructure. The color gradient transitions from a warm, yellowish core to a slightly bluer, fainter halo, indicative of a dominant population of older stars with potentially some ongoing, albeit subdued, star formation. The object appears somewhat elongated, suggesting it may not be perfectly spherical. There is no clear evidence of spiral arms or a distinct disk structure. The overall appearance is consistent with that of a mature galaxy, possibly undergoing minor interactions given some slight asymmetry in the outer regions.
