The galaxy presents as an elongated, elliptical structure, with a high degree of central concentration. The core region exhibits a bright, yellow-white hue, indicating a population of older stars. Moving outward from the core, the light intensity diminishes, with a subtle shift towards redder tones, possibly due to the presence of dust lanes or a slightly older stellar population in the outer regions. There are hints of blue along the edge of the galaxy, indicating the presence of star formation regions. The overall morphology appears relatively smooth and undisturbed.
