This galaxy presents as a largely elliptical or spheroidal structure, exhibiting a high degree of smoothness. The central region displays a concentrated luminosity, suggesting a significant stellar population and potentially an active galactic nucleus. The light appears to gradually fade as it extends outwards from the core. There are no discernible spiral arms or prominent dust lanes visible. There may be some slight asymmetry, but for the most part, it looks relaxed with no signs of recent interaction or major disturbances.
