The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core, gradually fading into a more diffuse outer halo. The color profile suggests an older stellar population, with a noticeable redder hue throughout the structure. There's no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of ongoing merger activity or major tidal distortions. The overall shape is nearly circular, indicating a low degree of ellipticity.
