The galaxy presents a largely smooth and rounded appearance. The central region exhibits a concentrated luminosity, appearing somewhat yellowish in color, which likely indicates an older stellar population. Surrounding the core, the galaxy displays a more diffuse halo, with hints of bluer tones in certain areas. This may suggest regions of ongoing star formation, though the rate appears relatively subdued. Overall, the galaxy lacks distinct structural features such as prominent spiral arms or a well-defined bar. Minor distortions cannot be ruled out, though the overall morphology suggests a system that has not recently undergone a major merger.
