The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge which radiates intensely with a yellow-white hue, suggesting a high density of older stars. The galaxy gradually diffuses outward from the center, transitioning from the yellow-white core to a more reddish color in its outer regions. This color gradient could indicate a lower metallicity and/or a slightly younger stellar population in these outer areas, or possibly dust reddening. Overall, the galaxy appears relatively undisturbed, with no obvious tidal tails, distortions or spiral arms. Its classification would suggest it's likely an elliptical galaxy, with a high probability of being relatively quiescent in terms of current star formation.
