The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. It appears nearly circular in projection. The central region exhibits a bright, yellowish hue, suggesting a population of older stars. The color becomes slightly redder in the outer regions of the galaxy but does not possess distinct spiral arms or bar structures. No significant tidal features or morphological disturbances are visible, indicating that the galaxy is not undergoing a major merger event. The smooth profile suggests a relatively high degree of order, likely composed of a dominant bulge component.
