The galaxy presents as a concentrated, elliptical morphology with a smooth light distribution. The central region is a bright, yellowish hue, suggestive of an older stellar population. There is a lack of discernible spiral arm structure or prominent dust lanes. Fainter, diffuse, greenish halos extend away from the central concentration, potentially indicating the presence of a more dispersed population of younger stars or ionized gas. Overall, the galaxy appears relatively undisturbed and quiescent.