The galaxy presents as an elliptical morphology, with a smooth, centralized concentration of light. The core region exhibits a yellowish hue, suggestive of an older stellar population. Extending outwards, a fainter, less defined halo surrounds the core, displaying a subtle transition in color towards redder tones, hinting at the presence of evolved stars. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. Overall, the galaxy appears to be a relatively undisturbed system, lacking any obvious signs of major recent merger activity or significant star formation.
