The galaxy appears as a luminous, elliptical-shaped structure. Its core exhibits a concentrated, bright yellowish-white hue, suggesting a high density of older stellar populations. The overall smooth and regular morphology indicates a relatively evolved system with minimal signs of recent major mergers or significant star formation activity, possibly due to morphological quenching. There appears to be a slight flattening. It has a hint of reddish glow, indicating the possible presence of dust, although not in significant quantities. The galaxy's profile suggests it is a well-defined system. The colors transition smoothly from the core to its edges.
