The galaxy presents a largely smooth morphology, appearing elliptical in shape. The central region exhibits a high concentration of luminosity, suggestive of an older stellar population. The color gradient transitions gradually from a yellowish-white core to a redder periphery. No prominent spiral arm structures or dust lanes are discernible, suggesting a lack of significant ongoing star formation. There is a subtle elongation, but no obvious signs of tidal disturbances or interactions with neighboring galaxies.
