The galaxy presents as a relatively smooth, centrally concentrated elliptical, exhibiting a notable lack of distinct structural features such as spiral arms or a prominent disk. The light profile appears to decline smoothly from the core outward. The central region is distinctly bright, with the intensity decreasing with radial distance, suggesting a high concentration of stars toward the galactic center. The color is generally yellowish, with the core being the most golden. Overall, the galaxy's morphology suggests a spheroid-dominated system, consistent with galaxies that are generally older and have ceased significant star formation in recent epochs. There is little evidence of ongoing merger activity or significant tidal disturbances.
