The galaxy presents as a luminous, elongated spheroid. It exhibits a smooth, featureless morphology with a concentrated central bulge. The color profile is predominantly yellow-white, indicating a population of older stars. There's a slight color gradient, transitioning from a warmer hue in the core to cooler, bluer tones in the outer regions. These blue tones may be due to younger stars. Overall, the galaxy shows no signs of significant disturbances or mergers.
