The galaxy presents as a largely smooth, elliptical structure. It exhibits a high degree of circularity, with a slight deviation towards a prolate shape not being ruled out. The central bulge appears prominent and intensely luminous, suggesting a high stellar density. The color profile indicates a relatively red population, with the luminosity concentrated towards the redder end of the spectrum. The isophotes are largely regular, without any obvious signs of significant tidal disturbances or ongoing major mergers. Subtle irregularities or minor disturbances within the galaxy are not apparent. The overall morphology indicates a lack of well-defined spiral arms or a prominent disk structure.
