The galaxy presents as a relatively smooth, centrally concentrated object with a nearly circular morphology. The light profile appears to be dominated by a bulge component, indicated by the smooth, elliptical isophotes and the concentration of light towards the galactic center. There is a noticeable color gradient, with the central region exhibiting a yellower hue suggestive of an older stellar population, while the outer regions appear slightly bluer, indicating the presence of younger stars or ongoing star formation. There is no significant evidence of spiral arms or a well-defined disk structure within the resolution limits of the image. No significant tidal features or signs of major mergers are observed, although there might be minor disturbances. The overall appearance suggests a galaxy transitioning toward a more quiescent state, with a dominant bulge and fading disk.
