The galaxy presents as a relatively smooth, centrally concentrated elliptical system, exhibiting a noticeable radial gradient in color and luminosity. The core region appears bright and exhibits a yellowish hue, suggesting a population of older, evolved stars. The color becomes gradually redder away from the center, possibly indicating a larger contribution of older stellar populations in the outer regions. 

There is no obvious evidence of spiral arm structures or significant dust lanes. The galaxy's morphology seems largely undisturbed. The slight ellipticity observed suggests that the galaxy is not perfectly spherical, though no major distortions are readily apparent. There are no signs of any major interaction or merging events.
