The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears round or nearly round. There is a diffuse halo extending outwards from the brighter central region of the galaxy; the colour of the central bulge region tends toward a more yellow-white hue, suggestive of an older stellar population. The outer regions exhibit a more bluish tint, indicating the presence of younger, hotter stars. No spiral arms, bar structures, or other distinct features are readily discernible in this image. The absence of significant morphological distortions suggests it is likely not undergoing a major merger event.
