This galaxy presents as a relatively smooth, centrally concentrated object. It appears mostly round in shape, showing minimal deviations from circular symmetry. The light distribution suggests a dominant bulge component, with a gradual decrease in intensity moving outwards from the center, with hints of disk features. There are no prominent spiral arms or distinct features suggesting ongoing major mergers or strong tidal interactions, however, there is a slightly disturbed feature, hinting at possible past interactions or minor mergers. The colors are generally consistent across the galaxy, with the bulge area appearing slightly brighter. Overall, it is likely an early-type spiral, leaning towards a smooth morphological classification.
