The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The radial color gradient transitions smoothly outwards from the core, with the outer regions appearing dimmer with a slight shift towards redder tones, potentially indicating an older stellar population or increased dust absorption. No distinct spiral arms, bars, or obvious signs of recent merger activity are discernible. Overall, the galaxy presents a regular, undisturbed structure.
