The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, tending towards a rounded appearance rather than being highly elongated. The central region shows a bright, intense luminosity, suggesting a significant concentration of stars. The color profile indicates a dominant yellowish-white hue, with minimal discernible blue tones, suggestive of a more evolved stellar population and reduced ongoing star formation. There are no prominent spiral arms or other well-defined structural features immediately apparent. There appears to be no significant major or minor disturbances. 