The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's light profile, exhibiting a yellow-gold hue, indicative of an older stellar population. The radial light distribution suggests a centrally concentrated mass. The outer regions appear fainter and less defined, with a slight elongation along one axis, hinting at a possible departure from perfect sphericity. No obvious spiral arm structure or significant dust lanes are apparent. Overall, the galaxy appears to be a relatively evolved system, possibly undergoing relatively little active star formation at the present epoch.
