The galaxy presents a largely smooth and elliptical morphology. A central bulge is readily apparent with a yellow-orange hue, indicating an older stellar population. Moving outward from the core, the light gradually diffuses, showing a transition to a fainter, less concentrated halo. There appears to be a slight flattening of the overall shape, moving away from being perfectly circular. No prominent spiral arm structures or dust lanes are visible, supporting the smooth classification. Faint hints of bluer light appear within the surrounding halo, hinting at ongoing, low-level star formation activity. There is no visual evidence of any major disturbances, mergers, or tidal tails. Overall, it appears to be a relatively isolated, evolved galaxy.
