The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an elliptical morphology, slightly elongated. The core of the galaxy is bright, exhibiting a bluish-white hue, suggesting the presence of a population of younger, hotter stars. There are hints of a faint disk or extension around the central bulge, but it is poorly defined. The color gradients appear subtle, with a gradual shift towards redder tones further from the core. Overall, the galaxy shows no signs of major disturbances or ongoing merging events, though some minor asymmetry could be present in its outer regions.
