The galaxy appears as a concentrated, elliptical-shaped object. The core presents a bright, yellowish hue, suggesting a population of older stars. There is a smooth gradient in luminosity moving outwards from the center, indicating a lack of significant dust lanes or spiral arm structures. The galaxy's overall structure seems relatively undisturbed with no indication of tidal tails or major distortions, hinting at a past without recent major merger events. A faint blue tinge is present in the outer edges, hinting at the possibility of some regions of ongoing or recent star formation. 
