The galaxy appears to be a relatively smooth and featureless elliptical galaxy. Its light is concentrated towards the center, with a gradual decrease in surface brightness towards the edges. The galaxy exhibits a slight elongation, deviating minimally from a perfectly circular shape. There is no apparent spiral structure, bar, or dust lane visible. Given the absence of prominent features, the galaxy likely has a low star formation rate, which is consistent with an older stellar population. The overall color is slightly redder, suggesting a dominance of older, redder stars. Faint disturbances are present along the edges, suggesting a potential merger event may have occurred.
