The galaxy appears as a relatively compact and well-defined elliptical. The light is concentrated towards the center, forming a bright, almost spherical nucleus, which suggests a high stellar density and potentially the presence of a supermassive black hole at its core. The galaxy exhibits a smooth, featureless morphology, with no discernible spiral arms or distinct dust lanes.

The color gradient suggests an older stellar population, with the central region exhibiting a yellowish-white hue, indicative of evolved stars. The outer regions gradually fade into a redder color, suggesting a population of older, cooler stars. Overall, the galaxy displays a high degree of rotational symmetry and appears undisturbed, without any obvious signs of recent mergers or interactions with other galaxies. Based on the apparent color and morphology, this galaxy likely has minimal ongoing star formation.
