The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth, featureless morphology in the visible spectrum. The light distribution suggests a high degree of radial symmetry, with intensity gradually decreasing from the core outwards. A slight elongation is observed, but the galaxy is predominantly round. No spiral arms or distinct disk features are discernible. The central region appears brighter and potentially more yellow compared to the outer regions, which suggests an older stellar population. There are no signs of active galactic nuclei, tidal tails, or other distortions indicative of recent merger events. A low level of ongoing star formation is potentially indicated by the color profile. The image implies that this galaxy is a relatively evolved and quiescent system.
