The galaxy presents as a lenticular or possibly an elliptical type, displaying a flattened, disk-like structure. A bright, concentrated central bulge dominates the galaxy's luminosity, suggesting a significant population of older stars residing within. The outer regions appear fainter and more diffuse with some evidence of spiral arms or dust lanes. The overall color is yellowish-white. There is no obvious evidence of active galactic nuclei activity or a recent major merger event. Overall, this appears to be a typical galaxy with ongoing or recently ceased star formation and a mass slightly above average.
