The galaxy presents an overall elliptical morphology, appearing somewhat elongated rather than perfectly circular. Its central region exhibits a high concentration of light, suggesting a prominent nucleus or bulge. The light distribution decreases gradually outwards from the center. A subtle reddish hue is observed within the core, potentially indicating an older stellar population. The overall color profile appears relatively uniform. There is a potential faint indication of spiral arms or tidal disturbances, though not definitive.
