The galaxy presents an elliptical morphology, elongated along its major axis. Its overall color profile suggests a relatively old stellar population, with a dominant yellowish-orange hue in the central regions. There is a gradual fading of color and intensity from the core outwards, with the outer edges exhibiting a more subdued, bluish tint. No prominent spiral arms or dust lanes are discernible. The galaxy appears smooth and relatively undisturbed, showing no obvious signs of ongoing major mergers or tidal interactions. The absence of distinct features indicates a lack of significant recent star formation activity.
