The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. There is little discernible structure, such as spiral arms or dust lanes, within the galaxy. The isophotes appear generally round, with no major distortions or tidal features indicative of recent merger activity. Fainter, bluer regions exist at the periphery, suggestive of a small amount of on-going star formation. The galaxy appears relatively isolated, with no immediately apparent companion galaxies or signs of significant gravitational interaction.