The galaxy presents as a generally elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a bright, yellowish hue, suggesting a population of older stars. There is a gradual decrease in surface brightness moving outwards from the core, with the outer regions appearing redder, indicating a potentially older stellar population or dust extinction. No distinct spiral arms or features are immediately apparent. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of recent merger activity or tidal distortions.
