The galaxy presents as a relatively smooth, elliptical object, displaying a high degree of central concentration. The core region appears bright and yellowish, suggesting an older stellar population. The luminosity gradually decreases with radial distance from the core. A subtle color gradient is observed, transitioning from the yellowish core to slightly bluer hues in the outer regions, possibly indicating some ongoing, though subdued, star formation at the fringes. Overall, the galaxy exhibits a well-defined, rounded morphology with no prominent features such as spiral arms or a distinct bar structure. There is no obvious sign of significant tidal disruption or ongoing merger activity, although faint asymmetries might indicate minor disturbances. The galaxy appears to be a moderately massive system.
