The galaxy presents a predominantly smooth morphology. It appears elliptical in shape, though with a slight flattening. The core exhibits a bright, concentrated luminosity, indicating a substantial stellar population density. The light gradually diffuses outward from the core, fading into the surrounding space. There is a hint of some internal structure or subtle features within the galaxy. Color gradients are observed, with a tendency toward redder hues in the central regions and bluer tones towards the outer edges, possibly indicating differences in stellar populations or dust content.
