The galaxy appears as a centrally concentrated object with a smooth light distribution. Its morphology is predominantly elliptical, exhibiting a nearly spherical shape with minimal discernible features such as spiral arms or a prominent disk structure. The galaxy's core is a bright, relatively compact region transitioning into a more diffuse halo. Color gradients are subtle but present, with the central region displaying a slightly yellower or redder hue compared to the outer regions, which appear bluer. There is no evidence of major tidal disturbances or ongoing mergers, and the overall structure suggests a system undergoing relatively quiescent evolution.
