The galaxy presents as a relatively smooth, elliptical structure. The central region displays a high concentration of light, indicating a prominent galactic nucleus. Moving outwards from the center, the light intensity gradually decreases. The overall shape deviates slightly from a perfect circle, appearing somewhat elongated or cigar-shaped. There is a hint of some features, possibly subtle spiral arms or dust lanes, although the resolution makes it difficult to discern definite structures. The color profile suggests a population of older stars. There is no evidence of significant ongoing star formation, supported by the relatively red colors and lack of bright blue regions typically associated with young, hot stars. Finally, there are no obvious signs of tidal tails or distortions, suggesting it is a relatively undisturbed system.
