The galaxy presents as a relatively smooth, centralized object. Its morphology appears largely elliptical, with a slight departure from perfect circularity, leaning towards an in-between or moderately elongated form. The light distribution is concentrated towards the center, indicating a prominent galactic bulge. The color profile suggests a higher concentration of older stars. There is no indication of significant spiral arm structures or active star formation regions visible in this image. The galaxy seems relatively undisturbed, with no clear evidence of ongoing or recent major mergers or tidal interactions.
