The galaxy presents a largely smooth and rounded morphology, indicating a relatively evolved system. There is a concentration of light in the center, suggesting a bulge component. The galaxy is approximately circular in shape, lacking any prominent spiral arms or bar structures. The central region exhibits a yellowish hue, which could be indicative of an older stellar population, while the outer regions appear slightly bluer, potentially suggesting ongoing or recent star formation. There is no obvious evidence of major mergers or significant tidal disturbances in the galaxy's structure, with the light distribution appearing relatively undisturbed and relaxed.
