The galaxy presents as a slightly elongated, smooth structure, consistent with an elliptical morphology. Its color gradient transitions from a bright, yellow-white core to a fainter, redder halo. There is no discernible spiral arm structure or dust lane features visible in the image. The galaxy exhibits a moderate degree of concentration, with the majority of its luminosity concentrated towards the center. The overall appearance suggests a galaxy with a relatively old stellar population and a low rate of current star formation activity. The morphology of the galaxy indicates that it is relatively undisturbed, with no major distortions that would indicate a recent merger or strong tidal interaction.