This galaxy presents as a centrally concentrated object with a fairly smooth morphology. There is a subtle elongation to its overall shape, suggesting it may be closer to an in-between elliptical than a perfectly spherical one. The core region exhibits a strong yellow hue, likely indicative of an older stellar population. The outer regions show a gradual decrease in intensity, with a slight shift toward redder tones, possibly reflecting the distribution of older, cooler stars away from the galactic center. There is a hint of very subtle, diffuse structure or a faint outer halo, but no prominent spiral arms or obvious signs of major disturbances are visible. There appear to be no signs of active merging events.
