This galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The light gradually diffuses outwards, indicating a decreasing stellar density toward the periphery. There's a distinct lack of readily identifiable spiral arm structures or prominent dust lanes. Its uniform appearance suggests it is a relatively evolved system with little ongoing star formation. The color profile appears relatively uniform, with a subtle shift towards redder hues in the central region. This reddening could be indicative of an older stellar population dominating the core. There are no obvious signs of recent mergers or tidal disturbances. The overall symmetry points to a dynamically relaxed system.
