The galaxy presents as a relatively smooth, centralized light distribution. It exhibits an elliptical morphology with high roundness, showing no obvious spiral arm structures or significant irregularities that would suggest an ongoing major merger event. The galaxy's color profile suggests a dominance of older stellar populations. A faint and subtle disk component might be present with slight color variations. The core region displays a concentrated, bright emission. There is minimal evidence of active star formation. The overall appearance points towards a fairly evolved system.
