The galaxy appears as a relatively smooth, centrally concentrated object with a slight degree of ellipticity. There's no prominent disk structure or spiral arms visible. The galaxy's color profile suggests a dominant population of older stars. The central region exhibits a concentration of light, possibly indicating the presence of a bulge. There are no obvious signs of recent major merger activity, though some minor disturbances cannot be ruled out. Based on the overall morphology, it is most likely an elliptical galaxy.