The galaxy presents as a well-defined elliptical shape with a smooth, centralized concentration of light. Its color profile suggests an older stellar population, appearing yellowish-orange towards the core. Moving outward from the center, there's a subtle transition to a bluer hue in the outer regions. This could indicate the presence of younger, bluer stars in the galactic outskirts or perhaps some degree of ongoing, though subdued, star formation activity. The overall structure appears undisturbed, showing no signs of major mergers or tidal disruptions. Faint dust lanes are not readily apparent, implying a relatively low gas and dust content. The galaxy exhibits a high degree of symmetry and lacks any prominent spiral arms or bar features.
