The galaxy presents as a largely smooth and elliptical structure. A bright central bulge dominates the overall light profile, with a relatively rapid decrease in luminosity moving outwards. The galaxy appears nearly spherical in shape, showing little evidence of a prominent disk component. There are no visible spiral arm structures or other distinct features typically associated with disk galaxies. Faint blue hues are visible in the outer regions, potentially indicating ongoing, albeit subdued, star formation. There is no clear indication of any major mergers or tidal disturbances. Overall, it seems to be a mature galaxy with a relatively high degree of central concentration.
