The galaxy presents an elliptical morphology, with a high degree of central concentration. The light profile appears smooth and relatively featureless across its extent. The color gradient suggests a population of older stars, shifting from a yellowish core to a slightly bluer halo. There is some evidence of a possible minor disturbance in the galaxy’s halo. The galaxy exhibits a moderate size. Overall, the galaxy appears to be an evolved system, likely with ongoing, low-level star formation.
