The galaxy appears to be a largely featureless elliptical galaxy with a smooth morphology. It exhibits a primarily round shape. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy's central bulge is bright and concentrated, gradually fading into the outer regions. There are no obvious signs of a major merger event, although some minor asymmetry or disturbance cannot be ruled out at this resolution. The color profile suggests a redder population, indicative of older stars.
