The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a bright core, which transitions smoothly into a more diffuse, extended halo. The color profile indicates a dominance of older stellar populations, with a yellowish-red hue. There is no clear evidence of spiral arms or significant dust lanes. The overall structure suggests a relatively relaxed system with little ongoing star formation. The galaxy appears largely undisturbed, showing no obvious signs of recent merger activity or tidal interactions. Its elongated shape indicates it is not perfectly spherical.
