The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish hue, indicative of an older stellar population. The surrounding halo appears fainter and more diffuse, with a slightly elongated shape, suggesting that it is not perfectly spherical. There is faint hint of a disk structure but no clearly visible spiral arms. There are no obvious signs of major mergers or significant tidal disturbances, although some minor asymmetry could indicate recent or ongoing interactions. The galaxy's red color suggests that it is a relatively passive galaxy with a low star formation rate. Overall, it appears to be a mature galaxy dominated by older stars.
