The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, exhibiting a high degree of circular symmetry. A prominent central bulge is observed, characterized by a yellowish-gold hue, suggesting an older stellar population. This bulge gradually fades into a surrounding halo of diffuse light. The halo displays a bluer tint, potentially indicating the presence of younger, hotter stars or ongoing star formation, although at a low rate. No distinct spiral arm structure or prominent dust lanes are apparent. There is little evidence of any significant tidal disturbances or interactions with other galaxies, suggesting the galaxy is relatively isolated and has not undergone a major merger event recently. The galaxy appears to be a massive galaxy with a stellar mass around 10^10 to 10^11 solar masses. The size is approximately 7-8 kpc in radius.
