The galaxy appears as a centrally concentrated, somewhat rounded structure. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a distinct bar. The central region displays a bright, concentrated core that gradually diffuses outward, with the galaxy's light decreasing steadily towards its periphery. The overall color profile suggests a population of older stars, with a slightly redder hue indicative of lower levels of recent star formation. There is a very slight suggestion of minor disturbances in the extended halo but this is a mostly isolated galaxy.
